This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA
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 08 03.1577 2461255.6577 12.75 23:46:50.97 +51:56:32.5
112.91674 -9.66899 galactic Cas Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:46:50.97 +51:56:32.5 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.038 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:50.97 +51:56:32.5: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:46:50.97 +51:56:32.5: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 46 50.97 +51 56 32.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.62 00:13:43.99 +54:31:40.9
117.42532 -7.94009 galactic Cas Second-epoch detections are separated by 2.1" 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 | target | 00:13:43.99 +54:31:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:43.99 +54:31:40.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:13:43.99 +54:31:40.9: 13.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 13 43.99 +54 31 40.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.53 23:56:31.16 +56:29:02.3
115.36545 -5.57883 galactic Cas Second-epoch detections are separated by 1.8" and 3.1 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 | 23:56:31.16 +56:29:02.3 (user input) | T | P | (position from user input) J-Ks=0.664+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:31.16 +56:29:02.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:56:31.16 +56:29:02.3: 13.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 56 31.16 +56 29 02.3 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.36 00:05:12.25 +51:03:42.6
115.55776 -11.14674 galactic Cas Second-epoch detections are separated by 0.4" 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 | target | 00:05:12.25 +51:03:42.6 (user input) | T | P | (position from user input) J-Ks=0.454+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:12.25 +51:03:42.6: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:05:12.25 +51:03:42.6: 13.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 05 12.25 +51 03 42.6 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.53 23:43:27.49 +50:48:57.4
112.10225 -10.62083 galactic Cas Second-epoch detections are separated by 2.1" and 4.0 pix
The object was found in VSX 2" Gaia DR3 1943850559784536064
Type: ROT
# Max. Min./Amp. JD0 Period
14.530 G 14.560 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:27.49 +50:48:57.4: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:43:27.49 +50:48:57.4: 13.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 43 27.49 +50 48 57.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943850559784536064,2461255.6577,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943850559784536064 20260803.1577 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.66 23:25:06.28 +54:08:56.6
110.40574 -6.60965 galactic Cas Second-epoch detections are separated by 2.1" and 3.3 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 J351.2592+54.1522 | 23:25:06.28 +54:08:56.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.423+/-0.038 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:06.28 +54:08:56.6: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:06.28 +54:08:56.6: 13.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 25 06.28 +54 08 56.6 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.2592+54.1522,2461255.6577,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.2592+54.1522 20260803.1577 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.53 23:31:29.79 +51:07:11.3
110.35774 -9.78978 galactic Cas Second-epoch detections are separated by 4.5" and 4.3 pix
The object was found in VSX21" Gaia DR3 1943300735250391552
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.820 G 13.850 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:29.79 +51:07:11.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:29.79 +51:07:11.3: 13.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 31 29.79 +51 07 11.3 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943300735250391552,2461255.6577,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943300735250391552 20260803.1577 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.47 23:44:15.73 +54:03:03.6
113.08032 -7.53085 galactic Cas Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:15.73 +54:03:03.6 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.045 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:15.73 +54:03:03.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:44:15.73 +54:03:03.6: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 44 15.73 +54 03 03.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.33 23:36:02.75 +51:05:47.2
111.04204 -10.02652 galactic Cas Second-epoch detections are separated by 0.6" and 3.6 pix
The object was found in VSX 1" Gaia DR3 1944763498032537728
Type: ROT
# Max. Min./Amp. JD0 Period
14.190 G 14.230 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:02.75 +51:05:47.2: 13.57 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:02.75 +51:05:47.2: 13.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.57 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 36 02.75 +51 05 47.2 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944763498032537728,2461255.6577,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944763498032537728 20260803.1577 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.52 00:09:51.69 +55:21:40.4
117.00115 -7.03104 galactic Cas Second-epoch detections are separated by 4.2" and 3.3 pix
The object was found in VSX 7" Gaia DR3 420635666616871808
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.930 G G
ATTENTION: measured mag 12.52 is 3.4 mag brighter than the VSX record maximum brightness 15.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:51.69 +55:21:40.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:09:51.69 +55:21:40.4: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 09 51.69 +55 21 40.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420635666616871808,2461255.6577,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420635666616871808 20260803.1577 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.53 23:44:35.93 +58:00:16.5
114.15040 -3.72304 galactic Cas Second-epoch detections are separated by 1.9" 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 | ATO J356.1503+58.0018 | 23:44:35.93 +58:00:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.889+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:35.93 +58:00:16.5: 13.42 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:44:35.93 +58:00:16.5: 13.65 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.42 +/- 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 08 03.1577* 23 44 35.93 +58 00 16.5 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.1503+58.0018,2461255.6577,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.1503+58.0018 20260803.1577 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.55 23:23:05.57 +54:06:19.4
110.11137 -6.55261 galactic Cas Second-epoch detections are separated by 6.0" 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 J350.7835+54.1050 | 23:23:05.57 +54:06:19.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:05.57 +54:06:19.4: 13.55 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:05.57 +54:06:19.4: 13.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.55 +/- 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 08 03.1577* 23 23 05.57 +54 06 19.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.7835+54.1050,2461255.6577,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.7835+54.1050 20260803.1577 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.62 23:19:48.01 +49:13:46.3
107.92556 -10.95365 galactic And Second-epoch detections are separated by 3.2" and 3.2 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 J349.9634+49.2319 | 23:19:48.01 +49:13:46.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.288+/-0.038 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:48.01 +49:13:46.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:48.01 +49:13:46.3: 13.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 19 48.01 +49 13 46.3 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.9634+49.2319,2461255.6577,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.9634+49.2319 20260803.1577 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.43 23:37:19.82 +57:11:47.8
112.99200 -4.23802 galactic Cas Second-epoch detections are separated by 3.7" and 2.7 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 J354.3318+57.1946 | 23:37:19.82 +57:11:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:19.82 +57:11:47.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:37:19.82 +57:11:47.8: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 37 19.82 +57 11 47.8 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.3318+57.1946,2461255.6577,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.3318+57.1946 20260803.1577 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.44 23:33:42.96 +53:40:49.7
111.47033 -7.45276 galactic Cas Second-epoch detections are separated by 2.9" and 2.9 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 | V1454 Cas | 23:33:46.88 +53:41:00.0 (Gaia DR3) | SRB (local) | 114.500000000000 (local) | Gaia3var=VARIABLE J-Ks=0.708+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:42.96 +53:40:49.7: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:33:42.96 +53:40:49.7: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 33 42.96 +53 40 49.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1454 Cas,2461255.6577,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1454 Cas 20260803.1577 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.51 23:21:44.29 +53:21:19.0
109.66504 -7.19014 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:21:44.29 +53:21:19.0 (user input) | T | P | (position from user input) J-Ks=0.706+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:44.29 +53:21:19.0: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:44.29 +53:21:19.0: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 21 44.29 +53 21 19.0 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.65 23:43:01.12 +51:44:15.3
112.28316 -9.71395 galactic Cas Second-epoch detections are separated by 3.1" and 3.5 pix
The object was found in VSX 2" ZTF J234300.97+514416.6
Type: BY
# Max. Min./Amp. JD0 Period
14.606 r Y 0.033 r 2458384.73580 7.262185600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:01.12 +51:44:15.3: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:43:01.12 +51:44:15.3: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 43 01.12 +51 44 15.3 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J234300.97+514416.6,2461255.6577,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J234300.97+514416.6 20260803.1577 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.69 23:30:19.86 +51:32:15.6
110.31387 -9.33603 galactic Cas Second-epoch detections are separated by 0.1" and 3.6 pix
The object was found in VSX 0" WISE J233019.8+513215
Type: EW
# Max. Min./Amp. JD0 Period
14.371 r Y 0.541 r 2458650.92960 0.304986000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:19.86 +51:32:15.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:19.86 +51:32:15.6: 13.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 19.86 +51 32 15.6 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J233019.8+513215,2461255.6577,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J233019.8+513215 20260803.1577 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.49 23:45:40.11 +49:42:46.8
112.15641 -11.77773 galactic Cas Second-epoch detections are separated by 4.9" and 3.9 pix
The object was found in VSX24" Gaia DR3 1943493321584730752
Type: VAR
# Max. Min./Amp. JD0 Period
13.710 G 13.760 G 0.169622000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:40.11 +49:42:46.8: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:45:40.11 +49:42:46.8: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 45 40.11 +49 42 46.8 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943493321584730752,2461255.6577,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943493321584730752 20260803.1577 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.53 23:26:34.69 +52:38:37.3
110.11801 -8.10394 galactic Cas Second-epoch detections are separated by 2.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:34.69 +52:38:37.3 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:34.69 +52:38:37.3: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:34.69 +52:38:37.3: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 26 34.69 +52 38 37.3 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.50 23:32:48.72 +55:10:10.9
111.79359 -5.99262 galactic Cas Second-epoch detections are separated by 2.1" and 3.6 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 1997429830128811008 | 23:32:49.13 +55:09:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.343+/-0.039 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:48.72 +55:10:10.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:32:48.72 +55:10:10.9: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 32 48.72 +55 10 10.9 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997429830128811008,2461255.6577,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997429830128811008 20260803.1577 12.50CV 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 08 03.1577 2461255.6577 12.63 23:18:56.86 +52:58:26.6
109.13615 -7.40236 galactic And Second-epoch detections are separated by 1.9" and 3.0 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 J349.7506+52.9663 | 23:18:56.86 +52:58:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.198+/-0.036 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.86 +52:58:26.6: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:56.86 +52:58:26.6: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 18 56.86 +52 58 26.6 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.7506+52.9663,2461255.6577,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.7506+52.9663 20260803.1577 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.30 00:04:18.17 +51:52:27.3
115.56883 -10.32236 galactic Cas Second-epoch detections are separated by 2.4" 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 | target | 00:04:18.17 +51:52:27.3 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:18.17 +51:52:27.3: 13.31 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:04:18.17 +51:52:27.3: 13.34 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 08 03.1577* 00 04 18.17 +51 52 27.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.30CV 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 08 03.1577 2461255.6577 12.46 23:41:04.22 +54:08:50.8
112.65117 -7.31373 galactic Cas Second-epoch detections are separated by 5.1" and 3.3 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 1994138991824060288 | 23:41:01.82 +54:09:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:04.22 +54:08:50.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:41:04.22 +54:08:50.8: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 41 04.22 +54 08 50.8 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994138991824060288,2461255.6577,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994138991824060288 20260803.1577 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.69 23:14:21.20 +52:49:14.4
108.42878 -7.29555 galactic And Second-epoch detections are separated by 3.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:14:21.20 +52:49:14.4 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.045 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:21.20 +52:49:14.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:21.20 +52:49:14.4: 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 08 03.1577* 23 14 21.20 +52 49 14.4 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.44 23:49:10.71 +51:58:44.7
113.27866 -9.72191 galactic Cas Second-epoch detections are separated by 1.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:49:10.71 +51:58:44.7 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.043 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:10.71 +51:58:44.7: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:49:10.71 +51:58:44.7: 13.91 +/- 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 08 03.1577* 23 49 10.71 +51 58 44.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.35 23:43:00.68 +55:31:09.9
113.29147 -6.06633 galactic Cas Second-epoch detections are separated by 4.4" and 2.6 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 1994511240927387776 | 23:43:02.02 +55:30:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:00.68 +55:31:09.9: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:43:00.68 +55:31:09.9: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 43 00.68 +55 31 09.9 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994511240927387776,2461255.6577,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994511240927387776 20260803.1577 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.34 23:43:58.95 +55:38:50.8
113.45832 -5.97863 galactic Cas Second-epoch detections are separated by 0.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:43:58.95 +55:38:50.8 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:58.95 +55:38:50.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:43:58.95 +55:38:50.8: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 43 58.95 +55 38 50.8 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.04 00:26:38.45 +56:47:19.5
119.52285 -5.91877 galactic Cas Second-epoch detections are separated by 0.9" 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 J006.6452+56.7887 | 00:26:38.45 +56:47:19.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.374+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:38.45 +56:47:19.5: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:26:38.45 +56:47:19.5: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 26 38.45 +56 47 19.5 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.6452+56.7887,2461255.6577,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.6452+56.7887 20260803.1577 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.61 23:23:49.35 +54:57:28.0
110.49912 -5.78504 galactic Cas Second-epoch detections are separated by 1.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:23:49.35 +54:57:28.0 (user input) | T | P | (position from user input) J-Ks=0.738+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:49.35 +54:57:28.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:49.35 +54:57:28.0: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 23 49.35 +54 57 28.0 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.31 23:34:26.31 +55:43:52.0
112.18294 -5.52539 galactic Cas Second-epoch detections are separated by 3.9" and 3.5 pix
The object was found in VSX 0" Gaia DR3 1997667152840867840
Type:
# Max. Min./Amp. JD0 Period
14.240 G 14.270 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:26.31 +55:43:52.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:26.31 +55:43:52.0: 13.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 34 26.31 +55 43 52.0 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997667152840867840,2461255.6577,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997667152840867840 20260803.1577 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.11 00:10:25.94 +58:05:06.9
117.51765 -4.35478 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 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 | 00:10:25.94 +58:05:06.9 (user input) | T | P | (position from user input) J-Ks=0.379+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:25.94 +58:05:06.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:10:25.94 +58:05:06.9: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 10 25.94 +58 05 06.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.35 23:14:57.96 +55:18:41.3
109.43210 -5.01142 galactic Cas Second-epoch detections are separated by 1.9" and 3.1 pix
The object was found in VSX 2" Gaia DR3 1997068640556377216
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.230 G 14.260 G 0.049653400000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:57.96 +55:18:41.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:57.96 +55:18:41.3: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 14 57.96 +55 18 41.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997068640556377216,2461255.6577,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997068640556377216 20260803.1577 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.39 23:20:01.49 +56:18:40.6
110.45541 -4.32999 galactic Cas Second-epoch detections are separated by 1.2" and 3.0 pix
The object was found in VSX24" ZTF J232001.54+561904.5
Type: RS
# Max. Min./Amp. JD0 Period
17.956 r Y 0.082 r 2458242.96660 0.228578100000
ATTENTION: measured mag 12.39 is 5.5 mag brighter than the VSX record maximum brightness 17.87 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:01.49 +56:18:40.6: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:01.49 +56:18:40.6: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 20 01.49 +56 18 40.6 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232001.54+561904.5,2461255.6577,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232001.54+561904.5 20260803.1577 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.30 23:40:38.95 +54:06:04.1
112.57861 -7.34150 galactic Cas Second-epoch detections are separated by 1.5" and 3.1 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 1994138167190364288 | 23:40:38.40 +54:05:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.180 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:38.95 +54:06:04.1: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:40:38.95 +54:06:04.1: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 40 38.95 +54 06 04.1 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994138167190364288,2461255.6577,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994138167190364288 20260803.1577 12.30CV 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 08 03.1577 2461255.6577 12.25 23:42:32.90 +58:08:11.3
113.92249 -3.52514 galactic Cas Second-epoch detections are separated by 1.7" and 3.2 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 J355.6365+58.1364 | 23:42:35.69 +58:08:11.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.338+/-0.050 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:32.90 +58:08:11.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:42:32.90 +58:08:11.3: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 42 32.90 +58 08 11.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.6365+58.1364,2461255.6577,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.6365+58.1364 20260803.1577 12.25CV 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 08 03.1577 2461255.6577 12.20 23:27:20.61 +49:42:14.3
109.26368 -10.92290 galactic And Second-epoch detections are separated by 0.4" and 3.7 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 | 23:27:20.61 +49:42:14.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:20.61 +49:42:14.3: 13.26 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:20.61 +49:42:14.3: 13.45 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 08 03.1577* 23 27 20.61 +49 42 14.3 12.2 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
target,2461255.6577,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.31 23:36:53.88 +55:39:27.7
112.49474 -5.69625 galactic Cas Second-epoch detections are separated by 2.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J354.2277+55.6571 | 23:36:53.88 +55:39:27.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.160+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:53.88 +55:39:27.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:53.88 +55:39:27.7: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 36 53.88 +55 39 27.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.2277+55.6571,2461255.6577,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.2277+55.6571 20260803.1577 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.23 23:44:34.08 +53:02:55.9
112.86240 -8.51053 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:34.08 +53:02:55.9 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:34.08 +53:02:55.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:44:34.08 +53:02:55.9: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 44 34.08 +53 02 55.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.07 23:30:56.68 +51:10:37.0
110.29220 -9.70865 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 23:30:56.68 +51:10:37.0 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:56.68 +51:10:37.0: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:56.68 +51:10:37.0: 13.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 56.68 +51 10 37.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.15 23:33:59.07 +52:15:29.4
111.08030 -8.82225 galactic Cas Second-epoch detections are separated by 3.4" 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 | ATO J353.4917+52.2587 | 23:34:00.73 +52:15:06.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:59.07 +52:15:29.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:33:59.07 +52:15:29.4: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 33 59.07 +52 15 29.4 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 J353.4917+52.2587,2461255.6577,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.4917+52.2587 20260803.1577 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.02 00:16:04.69 +54:40:19.5
117.78540 -7.84594 galactic Cas Second-epoch detections are separated by 0.8" and 3.8 pix
The object was found in VSX 6" Gaia DR3 419803954790045824
Type: RRC
# Max. Min./Amp. JD0 Period
20.030 G 20.620 G 0.328672000000
ATTENTION: measured mag 12.02 is 8.0 mag brighter than the VSX record maximum brightness 20.03 - 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-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:16:04.69 +54:40:19.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:16:04.69 +54:40:19.5: 13.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 16 04.69 +54 40 19.5 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419803954790045824,2461255.6577,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419803954790045824 20260803.1577 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 08 03.1577 2461255.6577 12.40 23:46:23.31 +57:38:21.1
114.28873 -4.13684 galactic Cas Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:46:23.31 +57:38:21.1 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.053 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:23.31 +57:38:21.1: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:46:23.31 +57:38:21.1: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 46 23.31 +57 38 21.1 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.26 23:08:56.46 +57:15:29.7
109.38746 -2.89330 galactic Cas Second-epoch detections are separated by 2.5" and 2.6 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 2009911348687087872 | 23:08:57.90 +57:15:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:08:56.46 +57:15:29.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:08:56.46 +57:15:29.7: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 08 56.46 +57 15 29.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009911348687087872,2461255.6577,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009911348687087872 20260803.1577 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.35 23:15:24.67 +54:15:49.6
109.10840 -6.01040 galactic Cas Second-epoch detections are separated by 3.0" and 3.1 pix
The object was found in VSX14" Gaia DR3 1996028536917159424
Type: ROT
# Max. Min./Amp. JD0 Period
15.260 G 15.320 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:24.67 +54:15:49.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:15:24.67 +54:15:49.6: 13.36 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 15 24.67 +54 15 49.6 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996028536917159424,2461255.6577,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996028536917159424 20260803.1577 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.27 23:14:20.68 +56:26:27.3
109.76526 -3.92841 galactic Cas Second-epoch detections are separated by 5.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.5813+56.4407 | 23:14:20.68 +56:26:27.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:20.68 +56:26:27.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:20.68 +56:26:27.3: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 14 20.68 +56 26 27.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.5813+56.4407,2461255.6577,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.5813+56.4407 20260803.1577 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.99 00:00:15.41 +57:43:09.0
116.11825 -4.47391 galactic Cas Second-epoch detections are separated by 1.2" and 3.5 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 | 00:00:15.41 +57:43:09.0 (user input) | T | P | (position from user input) J-Ks=0.857+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:15.41 +57:43:09.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:00:15.41 +57:43:09.0: 13.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 00 15.41 +57 43 09.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.99CV 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 08 03.1577 2461255.6577 12.23 23:26:03.13 +52:03:35.9
109.84865 -8.62945 galactic Cas Second-epoch detections are separated by 2.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:03.13 +52:03:35.9 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.041 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:03.13 +52:03:35.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:03.13 +52:03:35.9: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 26 03.13 +52 03 35.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.02 23:45:47.83 +57:16:15.9
114.11886 -4.47320 galactic Cas Second-epoch detections are separated by 3.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.4612+57.2675 | 23:45:47.83 +57:16:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.058 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.83 +57:16:15.9: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:45:47.83 +57:16:15.9: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 45 47.83 +57 16 15.9 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.4612+57.2675,2461255.6577,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.4612+57.2675 20260803.1577 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 08 03.1577 2461255.6577 12.06 23:31:09.82 +52:06:27.4
110.61711 -8.83431 galactic Cas Second-epoch detections are separated by 0.8" and 3.5 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 1991628016502919424 | 23:31:08.08 +52:06:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.544+/-0.060 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:09.82 +52:06:27.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:09.82 +52:06:27.4: 13.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 31 09.82 +52 06 27.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991628016502919424,2461255.6577,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991628016502919424 20260803.1577 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.26 23:16:41.18 +54:20:20.5
109.31015 -6.00755 galactic Cas Second-epoch detections are separated by 2.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:41.18 +54:20:20.5 (user input) | T | P | (position from user input) J-Ks=0.812+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:41.18 +54:20:20.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:41.18 +54:20:20.5: 13.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 16 41.18 +54 20 20.5 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.15 23:36:46.48 +53:03:10.3
111.72492 -8.18655 galactic Cas Second-epoch detections are separated by 0.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:36:46.48 +53:03:10.3 (user input) | T | P | (position from user input) J-Ks=0.620+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:46.48 +53:03:10.3: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:46.48 +53:03:10.3: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 36 46.48 +53 03 10.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.98 23:51:14.19 +53:29:30.8
113.94948 -8.32667 galactic Cas Second-epoch detections are separated by 3.9" 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 1993451109862397568 | 23:51:13.54 +53:29:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:14.19 +53:29:30.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:51:14.19 +53:29:30.8: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 51 14.19 +53 29 30.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993451109862397568,2461255.6577,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993451109862397568 20260803.1577 11.98CV 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 08 03.1577 2461255.6577 12.08 23:24:22.77 +57:21:09.2
111.37059 -3.55197 galactic Cas Second-epoch detections are separated by 1.7" and 2.9 pix
The object was found in VSX 2" Gaia DR3 2009364444729402112
Type: ROT
# Max. Min./Amp. JD0 Period
13.730 G 13.750 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:22.77 +57:21:09.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:22.77 +57:21:09.2: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 24 22.77 +57 21 09.2 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009364444729402112,2461255.6577,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009364444729402112 20260803.1577 12.08CV 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 08 03.1577 2461255.6577 12.09 23:10:31.41 +57:14:50.0
109.58122 -2.98537 galactic Cas Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:10:31.41 +57:14:50.0 (user input) | T | P | (position from user input) J-Ks=0.822+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:31.41 +57:14:50.0: 13.01 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:10:31.41 +57:14:50.0: 13.15 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 08 03.1577* 23 10 31.41 +57 14 50.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.97 23:48:45.32 +54:05:07.7
113.73277 -7.66292 galactic Cas Second-epoch detections are separated by 0.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:48:45.32 +54:05:07.7 (user input) | T | P | (position from user input) J-Ks=0.199+/-0.038 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:45.32 +54:05:07.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:48:45.32 +54:05:07.7: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 48 45.32 +54 05 07.7 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,2461255.6577,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.07 23:16:25.73 +52:40:53.5
108.67237 -7.53977 galactic And Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:25.73 +52:40:53.5 (user input) | T | P | (position from user input) J-Ks=0.185+/-0.044 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:25.73 +52:40:53.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:25.73 +52:40:53.5: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 16 25.73 +52 40 53.5 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.00 23:19:42.05 +51:36:25.9
108.75960 -8.72243 galactic And Second-epoch detections are separated by 1.9" and 3.1 pix
The object was found in VSX 1" ZTF J231942.15+513625.8
Type: DSCT
# Max. Min./Amp. JD0 Period
14.877 g Y 0.032 g 2458641.95080 0.061257100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:42.05 +51:36:25.9: 13.54 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:42.05 +51:36:25.9: 13.02 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 08 03.1577* 23 19 42.05 +51 36 25.9 12.0 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
ZTF J231942.15+513625.8,2461255.6577,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J231942.15+513625.8 20260803.1577 12.00CV 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 08 03.1577 2461255.6577 11.77 00:32:19.53 +57:14:54.2
120.33702 -5.52703 galactic Cas Second-epoch detections are separated by 0.1" and 3.8 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 421834546606595072 | 00:32:19.53 +57:14:54.2 (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)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:32:19.53 +57:14:54.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:32:19.53 +57:14:54.2: 13.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 32 19.53 +57 14 54.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 421834546606595072,2461255.6577,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 421834546606595072 20260803.1577 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.97 23:32:25.57 +51:54:36.9
110.74300 -9.08176 galactic Cas Second-epoch detections are separated by 0.1" and 3.6 pix
The object was found in VSX 0" Gaia DR3 1992931384459555584
Type: VAR
# Max. Min./Amp. JD0 Period
13.620 G 13.760 G 0.014758400000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:25.57 +51:54:36.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:32:25.57 +51:54:36.9: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 32 25.57 +51 54 36.9 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992931384459555584,2461255.6577,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992931384459555584 20260803.1577 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.14 23:16:35.53 +55:47:09.3
109.81963 -4.65243 galactic Cas Second-epoch detections are separated by 1.4" and 3.1 pix
The object was found in VSX16" Gaia DR3 1997099220723601536
Type: ROT
# Max. Min./Amp. JD0 Period
14.120 G 14.160 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:35.53 +55:47:09.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:35.53 +55:47:09.3: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 16 35.53 +55 47 09.3 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997099220723601536,2461255.6577,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997099220723601536 20260803.1577 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.14 23:12:31.74 +56:42:50.5
109.63370 -3.58219 galactic Cas Second-epoch detections are separated by 1.8" and 2.6 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 J348.1320+56.7184 | 23:12:31.74 +56:42:50.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.359+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:31.74 +56:42:50.5: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:31.74 +56:42:50.5: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 12 31.74 +56 42 50.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.1320+56.7184,2461255.6577,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.1320+56.7184 20260803.1577 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.95 23:45:04.37 +55:00:31.4
113.44345 -6.63574 galactic Cas Second-epoch detections are separated by 1.1" and 3.2 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 J356.2510+55.0071 | 23:45:01.72 +55:00:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.861+/-0.036 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:04.37 +55:00:31.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:45:04.37 +55:00:31.4: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 45 04.37 +55 00 31.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.2510+55.0071,2461255.6577,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.2510+55.0071 20260803.1577 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.90 23:27:29.39 +55:44:25.2
111.25104 -5.21591 galactic Cas Second-epoch detections are separated by 0.4" and 3.1 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 1996218129654164992 | 23:27:27.82 +55:43:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:29.39 +55:44:25.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:29.39 +55:44:25.2: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 27 29.39 +55 44 25.2 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
Gaia DR3 1996218129654164992,2461255.6577,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996218129654164992 20260803.1577 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 08 03.1577 2461255.6577 11.86 00:11:49.65 +56:14:26.5
117.41554 -6.20621 galactic Cas Second-epoch detections are separated by 1.1" 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 420781626786374144 | 00:11:47.32 +56:15:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.698+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:49.65 +56:14:26.5: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:11:49.65 +56:14:26.5: 13.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 11 49.65 +56 14 26.5 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420781626786374144,2461255.6577,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420781626786374144 20260803.1577 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.76 23:49:44.61 +55:38:29.7
114.24850 -6.18657 galactic Cas Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:49:44.61 +55:38:29.7 (user input) | T | P | (position from user input) J-Ks=0.679+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:44.61 +55:38:29.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:49:44.61 +55:38:29.7: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 49 44.61 +55 38 29.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.76CV 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 08 03.1577 2461255.6577 11.79 23:41:51.68 +54:39:58.9
112.90382 -6.84505 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 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 J355.4769+54.6722 | 23:41:51.68 +54:39:58.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:51.68 +54:39:58.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:41:51.68 +54:39:58.9: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 41 51.68 +54 39 58.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.4769+54.6722,2461255.6577,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.4769+54.6722 20260803.1577 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.62 23:35:14.12 +56:30:57.6
112.52056 -4.80754 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 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 1997767586357412736 | 23:35:15.42 +56:31:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.542+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:14.12 +56:30:57.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:35:14.12 +56:30:57.6: 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 08 03.1577* 23 35 14.12 +56 30 57.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997767586357412736,2461255.6577,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997767586357412736 20260803.1577 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 08 03.1577 2461255.6577 11.71 23:25:47.99 +52:39:36.7
110.01077 -8.04978 galactic And Second-epoch detections are separated by 0.3" and 3.5 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 1992495084501583616 | 23:25:50.01 +52:39:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.368+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:47.99 +52:39:36.7: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:47.99 +52:39:36.7: 13.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 25 47.99 +52 39 36.7 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992495084501583616,2461255.6577,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992495084501583616 20260803.1577 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 08 03.1577 2461255.6577 11.68 23:22:39.83 +57:01:55.9
111.04393 -3.77639 galactic Cas Second-epoch detections are separated by 0.3" and 2.9 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 J350.6835+57.0258 | 23:22:44.05 +57:01:33.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.793+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:39.83 +57:01:55.9: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:39.83 +57:01:55.9: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 22 39.83 +57 01 55.9 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.6835+57.0258,2461255.6577,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.6835+57.0258 20260803.1577 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 08 03.1577 2461255.6577 11.59 23:46:34.36 +57:42:58.1
114.33188 -4.06847 galactic Cas Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.6458+57.7147 | 23:46:34.36 +57:42:58.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.413+/-0.056 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:34.36 +57:42:58.1: 13.72 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:46:34.36 +57:42:58.1: 13.55 +/- 0.35 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 46 34.36 +57 42 58.1 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
ATO J356.6458+57.7147,2461255.6577,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.6458+57.7147 20260803.1577 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.69 23:15:55.87 +53:32:18.6
108.91499 -6.71393 galactic Cas Second-epoch detections are separated by 3.5" and 2.7 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 J348.9877+53.5276 | 23:15:55.87 +53:32:18.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:55.87 +53:32:18.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:15:55.87 +53:32:18.6: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 15 55.87 +53 32 18.6 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 J348.9877+53.5276,2461255.6577,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.9877+53.5276 20260803.1577 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.32 00:18:51.07 +50:04:25.7
117.58754 -12.45949 galactic Cas Second-epoch detections are separated by 2.4" and 4.1 pix
The object was found in VSX17" Gaia DR3 394501512170352128
Type: ROT
# Max. Min./Amp. JD0 Period
15.940 G 15.980 G K
ATTENTION: measured mag 11.32 is 4.6 mag brighter than the VSX record maximum brightness 15.94 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:51.07 +50:04:25.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:18:51.07 +50:04:25.7: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 18 51.07 +50 04 25.7 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 394501512170352128,2461255.6577,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394501512170352128 20260803.1577 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 08 03.1577 2461255.6577 11.64 23:17:56.22 +50:57:32.0
108.26594 -9.23096 galactic And Second-epoch detections are separated by 0.8" and 3.6 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 1991134163983802752 | 23:17:53.85 +50:57:18.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.338+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:56.22 +50:57:32.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:56.22 +50:57:32.0: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 17 56.22 +50 57 32.0 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991134163983802752,2461255.6577,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991134163983802752 20260803.1577 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 08 03.1577 2461255.6577 11.76 23:22:04.88 +53:49:28.0
109.87464 -6.76655 galactic Cas Second-epoch detections are separated by 1.9" and 3.5 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 J350.5204+53.8204 | 23:22:04.88 +53:49:28.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=11.490+/- (unrealisitic color!)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:04.88 +53:49:28.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:04.88 +53:49:28.0: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 22 04.88 +53 49 28.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.5204+53.8204,2461255.6577,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.5204+53.8204 20260803.1577 11.76CV 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 08 03.1577 2461255.6577 11.68 23:25:02.89 +56:51:11.0
111.29154 -4.05349 galactic Cas Second-epoch detections are separated by 1.4" and 3.1 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 | 23:25:02.89 +56:51:11.0 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.034 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:02.89 +56:51:11.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:02.89 +56:51:11.0: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 25 02.89 +56 51 11.0 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,2461255.6577,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 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 08 03.1577 2461255.6577 11.65 23:12:15.38 +56:31:13.1
109.52633 -3.74788 galactic Cas Second-epoch detections are separated by 1.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:12:15.38 +56:31:13.1 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=1.185+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:15.38 +56:31:13.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:15.38 +56:31:13.1: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 12 15.38 +56 31 13.1 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,2461255.6577,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.54 23:22:30.80 +52:04:54.8
109.33774 -8.42714 galactic And Second-epoch detections are separated by 0.5" 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 1992336857905747328 | 23:22:28.82 +52:04:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.729+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:30.80 +52:04:54.8: 12.76 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:30.80 +52:04:54.8: 12.68 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.71 +/- 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 08 03.1577* 23 22 30.80 +52 04 54.8 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
Gaia DR3 1992336857905747328,2461255.6577,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992336857905747328 20260803.1577 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.51 23:30:34.79 +51:52:37.3
110.45821 -9.02563 galactic Cas Second-epoch detections are separated by 0.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:34.79 +51:52:37.3 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:34.79 +51:52:37.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:34.79 +51:52:37.3: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 34.79 +51 52 37.3 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,2461255.6577,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.46 23:27:54.70 +55:41:49.2
111.29367 -5.27594 galactic Cas Second-epoch detections are separated by 0.8" and 3.2 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 1996218408825548672 | 23:27:55.29 +55:42:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.073+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:54.70 +55:41:49.2: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:54.70 +55:41:49.2: 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 08 03.1577* 23 27 54.70 +55 41 49.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996218408825548672,2461255.6577,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996218408825548672 20260803.1577 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 08 03.1577 2461255.6577 11.54 23:19:17.20 +52:37:40.5
109.06163 -7.74439 galactic And Second-epoch detections are separated by 0.5" and 3.4 pix
The object was found in VSX20" Gaia DR3 1992593800028520576
Type: ROT
# Max. Min./Amp. JD0 Period
13.530 G 13.570 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:17.20 +52:37:40.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:17.20 +52:37:40.5: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 19 17.20 +52 37 40.5 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
Gaia DR3 1992593800028520576,2461255.6577,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992593800028520576 20260803.1577 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.54 23:19:35.45 +54:16:30.4
109.68579 -6.21746 galactic Cas Second-epoch detections are separated by 3.2" and 2.7 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 1995993627422222976 | 23:19:35.56 +54:17:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.875+/-0.027 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:35.45 +54:16:30.4: 13.06 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:35.45 +54:16:30.4: 13.74 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.06 +/- 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 08 03.1577* 23 19 35.45 +54 16 30.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995993627422222976,2461255.6577,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995993627422222976 20260803.1577 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.33 23:40:37.12 +56:24:23.9
113.20579 -5.12189 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 pix
The object was found in VSX22" Gaia DR3 1997808405725291776
Type: RS
# Max. Min./Amp. JD0 Period
13.930 G 13.980 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:37.12 +56:24:23.9: 12.34 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:40:37.12 +56:24:23.9: 12.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 08 03.1577* 23 40 37.12 +56 24 23.9 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
Gaia DR3 1997808405725291776,2461255.6577,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997808405725291776 20260803.1577 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 08 03.1577 2461255.6577 11.64 23:17:17.48 +55:08:01.9
109.67820 -5.29675 galactic Cas Second-epoch detections are separated by 1.4" and 3.3 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 J349.3116+55.1290 | 23:17:17.48 +55:08:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.253+/-0.039 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:17.48 +55:08:01.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:17.48 +55:08:01.9: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 17 17.48 +55 08 01.9 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 J349.3116+55.1290,2461255.6577,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.3116+55.1290 20260803.1577 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 08 03.1577 2461255.6577 11.36 23:37:42.13 +52:46:09.3
111.77831 -8.49832 galactic Cas Second-epoch detections are separated by 0.8" and 3.7 pix
The object was found in VSX25" Gaia DR3 1993170871835982720
Type:
# Max. Min./Amp. JD0 Period
11.500 G 11.550 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:42.13 +52:46:09.3: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:37:42.13 +52:46:09.3: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 37 42.13 +52 46 09.3 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 1993170871835982720,2461255.6577,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993170871835982720 20260803.1577 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 08 03.1577 2461255.6577 11.39 23:23:04.22 +52:29:55.9
109.56163 -8.06378 galactic And Second-epoch detections are separated by 1.7" and 3.2 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 1992412483690187776 | 23:23:04.96 +52:29:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.177+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:04.22 +52:29:55.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:04.22 +52:29:55.9: 13.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 23 04.22 +52 29 55.9 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992412483690187776,2461255.6577,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992412483690187776 20260803.1577 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 08 03.1577 2461255.6577 11.41 23:13:33.87 +53:34:52.7
108.60167 -6.54517 galactic Cas Second-epoch detections are separated by 0.4" and 3.1 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 1995573094286898944 | 23:13:35.10 +53:34:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.132+/-0.033 (A)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:33.87 +53:34:52.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:13:33.87 +53:34:52.7: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 13 33.87 +53 34 52.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995573094286898944,2461255.6577,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995573094286898944 20260803.1577 11.41CV 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 08 03.1577 2461255.6577 11.39 23:16:55.84 +55:40:34.4
109.82481 -4.77192 galactic Cas Second-epoch detections are separated by 0.6" and 3.1 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 J349.2418+55.6751 | 23:16:59.12 +55:40:23.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.648+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:55.84 +55:40:34.4: 13.40 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:55.84 +55:40:34.4: 13.62 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.40 +/- 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 08 03.1577* 23 16 55.84 +55 40 34.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.2418+55.6751,2461255.6577,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.2418+55.6751 20260803.1577 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 08 03.1577 2461255.6577 11.23 23:39:41.70 +57:16:05.3
113.32010 -4.25867 galactic Cas Second-epoch detections are separated by 3.0" and 3.1 pix
The object was found in VSX19" Gaia DR3 1998666952508357760
Type: ROT
# Max. Min./Amp. JD0 Period
14.090 G 14.120 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:41.70 +57:16:05.3: 13.60 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:39:41.70 +57:16:05.3: 13.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.60 +/- 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 08 03.1577* 23 39 41.70 +57 16 05.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998666952508357760,2461255.6577,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998666952508357760 20260803.1577 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 08 03.1577 2461255.6577 11.29 23:29:51.32 +56:20:02.2
111.75380 -4.75694 galactic Cas Second-epoch detections are separated by 0.7" and 3.0 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 1998497181033243520 | 23:29:53.89 +56:19:55.6 (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) J-Ks=0.864+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:51.32 +56:20:02.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:29:51.32 +56:20:02.2: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 29 51.32 +56 20 02.2 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
Large-amplitude variable Gaia DR2 1998497181033243520,2461255.6577,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1998497181033243520 20260803.1577 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 08 03.1577 2461255.6577 11.38 23:18:41.24 +54:16:19.5
109.56049 -6.17402 galactic Cas Second-epoch detections are separated by 1.5" 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 1995973075999277440 | 23:18:38.04 +54:16:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.721+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:41.24 +54:16:19.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:41.24 +54:16:19.5: 13.72 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 08 03.1577* 23 18 41.24 +54 16 19.5 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995973075999277440,2461255.6577,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995973075999277440 20260803.1577 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 08 03.1577 2461255.6577 10.98 23:46:43.16 +50:45:04.7
112.59202 -10.81656 galactic Cas Second-epoch detections are separated by 1.8" 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 1944165707304891264 | 23:46:44.50 +50:45:28.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.505+/-0.034 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:43.16 +50:45:04.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:46:43.16 +50:45:04.7: 13.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 46 43.16 +50 45 04.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944165707304891264,2461255.6577,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944165707304891264 20260803.1577 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 08 03.1577 2461255.6577 11.05 23:28:05.73 +55:31:17.7
111.26231 -5.45050 galactic Cas Second-epoch detections are separated by 7.6" 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 | ATO J352.0252+55.5206 | 23:28:06.19 +55:31:54.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:05.73 +55:31:17.7: 12.36 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:05.73 +55:31:17.7: 12.58 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 08 03.1577* 23 28 05.73 +55 31 17.7 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 J352.0252+55.5206,2461255.6577,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.0252+55.5206 20260803.1577 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 08 03.1577 2461255.6577 11.16 23:20:50.24 +57:13:06.3
110.87385 -3.51696 galactic Cas Second-epoch detections are separated by 1.0" and 2.9 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 2009382964622103680 | 23:20:48.14 +57:12:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.262+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:50.24 +57:13:06.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:50.24 +57:13:06.3: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 20 50.24 +57 13 06.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009382964622103680,2461255.6577,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009382964622103680 20260803.1577 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 08 03.1577 2461255.6577 11.34 23:12:44.76 +54:33:22.2
108.85445 -5.59565 galactic Cas Second-epoch detections are separated by 2.2" 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 1996470055253780096 | 23:12:42.20 +54:33:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=0.953+/-0.032 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:44.76 +54:33:22.2: 13.24 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:44.76 +54:33:22.2: 13.44 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.24 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 12 44.76 +54 33 22.2 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 1996470055253780096,2461255.6577,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996470055253780096 20260803.1577 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.20 23:17:35.31 +54:08:15.4
109.36141 -6.24281 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J349.4060+54.1166 | 23:17:37.25 +54:07:40.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:35.31 +54:08:15.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:35.31 +54:08:15.4: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 17 35.31 +54 08 15.4 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
ATO J349.4060+54.1166,2461255.6577,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.4060+54.1166 20260803.1577 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 08 03.1577 2461255.6577 10.93 23:56:33.04 +56:44:30.9
115.42465 -5.32767 galactic Cas Second-epoch detections are separated by 3.3" and 3.0 pix
The object was found in VSX15" V0874 Cas
Type: EA
# Max. Min./Amp. JD0 Period
13.980 V 14.310 V 2449904.93000 1.200070000000
ATTENTION: measured mag 10.93 is 3.1 mag brighter than the VSX record maximum brightness 13.98 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:33.04 +56:44:30.9: 12.80 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:56:33.04 +56:44:30.9: 12.76 +/- 0.22 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 08 03.1577* 23 56 33.04 +56 44 30.9 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
V0874 Cas,2461255.6577,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0874 Cas 20260803.1577 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 08 03.1577 2461255.6577 11.18 23:12:41.15 +54:49:13.2
108.94542 -5.34733 galactic Cas Second-epoch detections are separated by 1.7" and 3.2 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 1996494626770732160 | 23:12:37.83 +54:49:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.15 +54:49:13.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:41.15 +54:49:13.2: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 12 41.15 +54 49 13.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996494626770732160,2461255.6577,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996494626770732160 20260803.1577 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 10.98 23:18:56.50 +53:20:37.9
109.26663 -7.05595 galactic Cas Second-epoch detections are separated by 1.1" and 3.4 pix
The object was found in VSX 1" Gaia DR3 1995687275993223168
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.50 +53:20:37.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:56.50 +53:20:37.9: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 18 56.50 +53 20 37.9 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 1995687275993223168,2461255.6577,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995687275993223168 20260803.1577 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 08 03.1577 2461255.6577 10.70 23:37:54.62 +52:32:03.2
111.74136 -8.73262 galactic Cas Second-epoch detections are separated by 0.5" and 3.7 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 J354.4870+52.5413 | 23:37:56.31 +52:32:16.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.573+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:54.62 +52:32:03.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:37:54.62 +52:32:03.2: 13.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 37 54.62 +52 32 03.2 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
ATO J354.4870+52.5413,2461255.6577,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.4870+52.5413 20260803.1577 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 08 03.1577 2461255.6577 10.80 23:21:14.39 +55:23:14.2
110.29643 -5.25614 galactic Cas Second-epoch detections are separated by 0.6" and 3.0 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 1996852414723764608 | 23:21:11.12 +55:23:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.546+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:14.39 +55:23:14.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:14.39 +55:23:14.2: 13.64 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 08 03.1577* 23 21 14.39 +55 23 14.2 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 1996852414723764608,2461255.6577,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996852414723764608 20260803.1577 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 08 03.1577 2461255.6577 10.88 23:11:10.96 +55:59:33.2
109.18892 -4.18083 galactic Cas Second-epoch detections are separated by 1.1" and 3.1 pix
The object was found in VSX25" ZTF J231108.03+555931.6
Type: EA
# Max. Min./Amp. JD0 Period
15.753 r Y 0.151 r 2458335.86160 0.819205200000
ATTENTION: measured mag 10.88 is 4.7 mag brighter than the VSX record maximum brightness 15.60 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:10.96 +55:59:33.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:11:10.96 +55:59:33.2: 13.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 11 10.96 +55 59 33.2 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
ZTF J231108.03+555931.6,2461255.6577,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231108.03+555931.6 20260803.1577 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 08 03.1577 2461255.6577 10.57 23:38:08.00 +53:36:18.4
112.08021 -7.71505 galactic Cas Second-epoch detections are separated by 0.5" 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 1994109575585917056 | 23:38:05.75 +53:36:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.246+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:08.00 +53:36:18.4: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:38:08.00 +53:36:18.4: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 38 08.00 +53 36 18.4 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 1994109575585917056,2461255.6577,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994109575585917056 20260803.1577 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 08 03.1577 2461255.6577 10.47 23:19:15.91 +51:56:02.6
108.81197 -8.39274 galactic And Second-epoch detections are separated by 1.7" and 3.7 pix
The object was found in VSX 1" Gaia DR3 1992357714266211328
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.290 G 12.320 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:15.91 +51:56:02.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:15.91 +51:56:02.6: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 19 15.91 +51 56 02.6 10.5 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
Gaia DR3 1992357714266211328,2461255.6577,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992357714266211328 20260803.1577 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 08 03.1577 2461255.6577 10.24 23:50:25.76 +49:51:14.2
112.95267 -11.83200 galactic Cas Second-epoch detections are separated by 0.9" 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 1940880469640450304 | 23:50:26.96 +49:51:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.045+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:25.76 +49:51:14.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:50:25.76 +49:51:14.2: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 50 25.76 +49 51 14.2 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 1940880469640450304,2461255.6577,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940880469640450304 20260803.1577 10.24CV 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 08 03.1577 2461255.6577 10.42 23:31:12.57 +53:30:57.7
111.06265 -7.49670 galactic Cas Second-epoch detections are separated by 0.6" 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 1994058620093865984 | 23:31:12.65 +53:30:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:12.57 +53:30:57.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:12.57 +53:30:57.7: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 31 12.57 +53 30 57.7 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 1994058620093865984,2461255.6577,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994058620093865984 20260803.1577 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 08 03.1577 2461255.6577 10.32 23:31:08.95 +54:16:09.2
111.28771 -6.77732 galactic Cas Second-epoch detections are separated by 0.1" and 3.3 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 | Large-amplitude variable Gaia DR2 1994340477332018432 | 23:31:09.41 +54:16:29.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.319+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:08.95 +54:16:09.2: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:08.95 +54:16:09.2: 13.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 31 08.95 +54 16 09.2 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
Large-amplitude variable Gaia DR2 1994340477332018432,2461255.6577,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1994340477332018432 20260803.1577 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 08 03.1577 2461255.6577 10.00 23:36:32.69 +50:40:34.5
110.99418 -10.45142 galactic And Second-epoch detections are separated by 0.4" and 3.7 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 1944540365891633792 | 23:36:31.17 +50:40:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.036+/-0.047 (A)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:32.69 +50:40:34.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:32.69 +50:40:34.5: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 36 32.69 +50 40 34.5 10.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944540365891633792,2461255.6577,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944540365891633792 20260803.1577 10.00CV 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 08 03.1577 2461255.6577 10.13 23:23:09.38 +56:38:52.8
110.97807 -4.16087 galactic Cas Second-epoch detections are separated by 0.8" and 3.1 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 1997288542883461248 | 23:23:07.27 +56:38:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:09.38 +56:38:52.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:09.38 +56:38:52.8: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 23 09.38 +56 38 52.8 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 1997288542883461248,2461255.6577,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997288542883461248 20260803.1577 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 08 03.1577 2461255.6577 9.07 23:15:52.45 +52:57:57.3
108.69757 -7.24435 galactic And Second-epoch detections are separated by 1.7" and 3.5 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 J348.9601+52.9506 | 23:15:51.87 +52:57:37.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1927AnHar.100...33C HD 236076
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:52.45 +52:57:57.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:15:52.45 +52:57:57.3: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 15 52.45 +52 57 57.3 9.1 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
ATO J348.9601+52.9506,2461255.6577,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.9601+52.9506 20260803.1577 9.07CV 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 08 03.1577 2461255.6577 9.41 23:21:37.62 +55:42:58.8
110.46106 -4.96565 galactic Cas Second-epoch detections are separated by 0.8" and 3.0 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 1997000745714549504 | 23:21:40.22 +55:42:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:37.62 +55:42:58.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:37.62 +55:42:58.8: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 21 37.62 +55 42 58.8 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 1997000745714549504,2461255.6577,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997000745714549504 20260803.1577 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 08 03.1577 2461255.6577 9.87 23:26:05.79 +53:11:06.1
110.22685 -7.56851 galactic Cas Second-epoch detections are separated by 0.7" and 3.3 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 J351.5243+53.1850 | 23:26:05.85 +53:11:06.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.187+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:05.79 +53:11:06.1: 12.35 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:05.79 +53:11:06.1: 12.33 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 08 03.1577* 23 26 05.79 +53 11 06.1 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.5243+53.1850,2461255.6577,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.5243+53.1850 20260803.1577 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 08 03.1577 2461255.6577 10.62 23:27:06.61 +56:40:02.3
111.49903 -4.32093 galactic Cas Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was found in ASASSN-V 1" ASASSN-V J232706.67+564001.6
Type: L
MeanMag 12.94 m Amp. 0.12 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:06.61 +56:40:02.3: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:06.61 +56:40:02.3: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 27 06.61 +56 40 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
VARIABLE_NAME,2461255.6577,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1577 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 08 03.1577 2461255.6577 10.70 23:26:19.35 +51:13:14.5
109.61043 -9.43617 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 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 1991384509038443904 | 23:26:16.19 +51:12:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:19.35 +51:13:14.5: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:19.35 +51:13:14.5: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 26 19.35 +51 13 14.5 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 1991384509038443904,2461255.6577,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991384509038443904 20260803.1577 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 08 03.1577 2461255.6577 10.79 23:19:40.15 +50:08:15.6
108.23111 -10.09637 galactic And Second-epoch detections are separated by 1.4" and 3.7 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 1991224633173822464 | 23:19:40.56 +50:07:35.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 1958PMcCO..13b....V AG+49 2086
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:40.15 +50:08:15.6: 13.17 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:40.15 +50:08:15.6: 13.72 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.17 +/- 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 08 03.1577* 23 19 40.15 +50 08 15.6 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991224633173822464,2461255.6577,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991224633173822464 20260803.1577 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 08 03.1577 2461255.6577 10.87 23:22:36.51 +57:23:01.3
111.15553 -3.44292 galactic Cas Second-epoch detections are separated by 1.7" and 3.0 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 2009390970447326080 | 23:22:32.69 +57:22:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.745+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:36.51 +57:23:01.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:36.51 +57:23:01.3: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 22 36.51 +57 23 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 2009390970447326080,2461255.6577,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009390970447326080 20260803.1577 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 08 03.1577 2461255.6577 10.92 23:25:41.45 +55:09:05.3
110.81721 -5.69059 galactic Cas Second-epoch detections are separated by 0.7" and 3.2 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 1996185664003851520 | 23:25:37.96 +55:09:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:41.45 +55:09:05.3: 12.05 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:41.45 +55:09:05.3: 11.92 +/- 0.09 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 25 41.45 +55 09 05.3 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 1996185664003851520,2461255.6577,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996185664003851520 20260803.1577 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 08 03.1577 2461255.6577 11.21 23:13:38.70 +53:34:21.6
108.60962 -6.55762 galactic Cas Second-epoch detections are separated by 1.2" and 3.2 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 1995573094286898944 | 23:13:35.10 +53:34:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.475+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:38.70 +53:34:21.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:13:38.70 +53:34:21.6: 13.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 13 38.70 +53 34 21.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995573094286898944,2461255.6577,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995573094286898944 20260803.1577 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 08 03.1577 2461255.6577 11.08 23:29:11.90 +53:11:19.2
110.67203 -7.71423 galactic Cas Second-epoch detections are separated by 1.4" and 3.6 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 1992540782954086144 | 23:29:14.93 +53:11:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:11.90 +53:11:19.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:29:11.90 +53:11:19.2: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 29 11.90 +53 11 19.2 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 1992540782954086144,2461255.6577,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992540782954086144 20260803.1577 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 08 03.1577 2461255.6577 11.21 23:28:27.08 +51:42:39.1
110.08889 -9.07954 galactic Cas Second-epoch detections are separated by 0.3" and 3.6 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 1991589086918724480 | 23:28:26.77 +51:42:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:27.08 +51:42:39.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:27.08 +51:42:39.1: 13.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 28 27.08 +51 42 39.1 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 1991589086918724480,2461255.6577,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991589086918724480 20260803.1577 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 08 03.1577 2461255.6577 11.15 23:58:05.32 +56:28:01.7
115.57482 -5.64064 galactic Cas Second-epoch detections are separated by 1.4" and 3.5 pix
The object was found in VSX 1" ASASSN-V J235805.40+562800.5
Type: YSO
# Max. Min./Amp. JD0 Period
13.410 V 13.540 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:05.32 +56:28:01.7: 12.29 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:58:05.32 +56:28:01.7: 12.49 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 08 03.1577* 23 58 05.32 +56 28 01.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235805.40+562800.5,2461255.6577,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235805.40+562800.5 20260803.1577 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 08 03.1577 2461255.6577 11.38 23:16:50.72 +52:05:37.3
108.51793 -8.11089 galactic And Second-epoch detections are separated by 1.0" and 3.2 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 J349.1851+52.0807 | 23:16:46.44 +52:05:23.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.402+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:50.72 +52:05:37.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:50.72 +52:05:37.3: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 16 50.72 +52 05 37.3 11.4 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 J349.1851+52.0807,2461255.6577,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.1851+52.0807 20260803.1577 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 08 03.1577 2461255.6577 11.27 23:34:22.93 +53:50:20.2
111.61264 -7.33073 galactic Cas Second-epoch detections are separated by 0.7" and 3.5 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 1994092400019847168 | 23:34:27.25 +53:50:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:22.93 +53:50:20.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:22.93 +53:50:20.2: 13.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 34 22.93 +53 50 20.2 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 1994092400019847168,2461255.6577,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994092400019847168 20260803.1577 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 08 03.1577 2461255.6577 11.47 23:23:47.56 +54:34:21.7
110.36577 -6.14659 galactic Cas Second-epoch detections are separated by 0.8" and 3.3 pix
The object was found in VSX 0" ZTF J232347.55+543421.8
Type: SR
# Max. Min./Amp. JD0 Period
12.954 r Y 0.042 r 2458657.89370 34.975481300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:47.56 +54:34:21.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:47.56 +54:34:21.7: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 23 47.56 +54 34 21.7 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
ZTF J232347.55+543421.8,2461255.6577,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232347.55+543421.8 20260803.1577 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.41 23:31:35.90 +53:08:29.6
111.00229 -7.87089 galactic Cas Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:35.90 +53:08:29.6 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:35.90 +53:08:29.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:35.90 +53:08:29.6: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 31 35.90 +53 08 29.6 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,2461255.6577,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.41CV 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 08 03.1577 2461255.6577 11.57 23:25:28.04 +49:20:13.5
108.84779 -11.16928 galactic And Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:28.04 +49:20:13.5 (user input) | T | P | (position from user input) J-Ks=0.648+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.04 +49:20:13.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:28.04 +49:20:13.5: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 25 28.04 +49 20 13.5 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 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 08 03.1577 2461255.6577 11.51 23:43:15.02 +51:40:39.5
112.30214 -9.78126 galactic Cas Second-epoch detections are separated by 0.3" and 3.7 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 1944699245322764544 | 23:43:17.97 +51:41:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.348+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:15.02 +51:40:39.5: 12.92 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:43:15.02 +51:40:39.5: 12.97 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 08 03.1577* 23 43 15.02 +51 40 39.5 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944699245322764544,2461255.6577,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944699245322764544 20260803.1577 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.70 23:16:38.05 +55:10:33.8
109.60536 -5.22374 galactic Cas Second-epoch detections are separated by 2.7" 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 1996869109257874304 | 23:16:38.55 +55:09:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.018+/-0.031 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:38.05 +55:10:33.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:38.05 +55:10:33.8: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 16 38.05 +55 10 33.8 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
Gaia DR3 1996869109257874304,2461255.6577,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996869109257874304 20260803.1577 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.60 23:30:32.18 +49:52:18.7
109.81565 -10.92834 galactic And Second-epoch detections are separated by 0.7" and 3.7 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 J352.6481+49.8736 | 23:30:33.67 +49:52:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.333+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:32.18 +49:52:18.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:32.18 +49:52:18.7: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 32.18 +49 52 18.7 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.6481+49.8736,2461255.6577,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.6481+49.8736 20260803.1577 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 08 03.1577 2461255.6577 11.56 23:50:05.36 +50:49:19.3
113.13538 -10.87909 galactic Cas Second-epoch detections are separated by 2.0" 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 | Gaia DR3 1943993874253244032 | 23:50:02.21 +50:49:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1927AnHar.100...33C HD 236225 J-Ks=0.876+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:05.36 +50:49:19.3: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:50:05.36 +50:49:19.3: 13.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 50 05.36 +50 49 19.3 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943993874253244032,2461255.6577,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943993874253244032 20260803.1577 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.78 23:26:00.27 +52:50:48.1
110.10202 -7.88372 galactic Cas Second-epoch detections are separated by 0.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:00.27 +52:50:48.1 (user input) | T | P | (position from user input) J-Ks=0.773+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:00.27 +52:50:48.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:00.27 +52:50:48.1: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 26 00.27 +52 50 48.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.78CV 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 08 03.1577 2461255.6577 11.71 23:29:24.24 +51:40:00.7
110.21654 -9.16815 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 | 23:29:24.24 +51:40:00.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.24 +51:40:00.7: 13.09 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:29:24.24 +51:40:00.7: 13.01 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 08 03.1577* 23 29 24.24 +51 40 00.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 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 08 03.1577 2461255.6577 11.71 23:34:39.79 +51:08:28.0
110.84486 -9.91994 galactic Cas Second-epoch detections are separated by 0.9" and 3.8 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 J353.6504+51.1309 | 23:34:39.55 +51:07:48.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:39.79 +51:08:28.0: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:39.79 +51:08:28.0: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 34 39.79 +51 08 28.0 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
ATO J353.6504+51.1309,2461255.6577,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.6504+51.1309 20260803.1577 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 08 03.1577 2461255.6577 11.67 23:33:10.17 +56:17:31.8
112.18020 -4.93698 galactic Cas Second-epoch detections are separated by 1.9" and 3.4 pix
The object was found in VSX 1" Gaia DR3 1997756522521467008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.600 G 13.640 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:10.17 +56:17:31.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:33:10.17 +56:17:31.8: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 33 10.17 +56 17 31.8 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
Gaia DR3 1997756522521467008,2461255.6577,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997756522521467008 20260803.1577 11.67CV 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 08 03.1577 2461255.6577 11.91 23:11:51.57 +55:18:28.9
109.01875 -4.85084 galactic Cas Second-epoch detections are separated by 0.5" and 3.1 pix
The object was found in VSX 4" Gaia DR3 1996757100812082688
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.560 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.57 +55:18:28.9: 13.61 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:11:51.57 +55:18:28.9: 13.64 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.61 +/- 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 08 03.1577* 23 11 51.57 +55 18 28.9 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996757100812082688,2461255.6577,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996757100812082688 20260803.1577 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.90 23:24:46.31 +54:53:45.7
110.60782 -5.88857 galactic Cas Second-epoch detections are separated by 1.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:46.31 +54:53:45.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.667+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:46.31 +54:53:45.7: 12.99 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:46.31 +54:53:45.7: 12.96 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 08 03.1577* 23 24 46.31 +54 53 45.7 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,2461255.6577,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 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 08 03.1577 2461255.6577 11.93 23:17:29.43 +52:31:58.8
108.77019 -7.73634 galactic And Second-epoch detections are separated by 3.8" and 3.7 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 1992633451161006720 | 23:17:33.26 +52:31:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.271+/-0.044 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:29.43 +52:31:58.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:29.43 +52:31:58.8: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 17 29.43 +52 31 58.8 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992633451161006720,2461255.6577,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992633451161006720 20260803.1577 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.01 23:16:56.04 +51:46:16.2
108.41330 -8.41665 galactic And Second-epoch detections are separated by 2.4" and 3.5 pix
The object was found in VSX25" Gaia DR3 1991990683541947776
Type:
# Max. Min./Amp. JD0 Period
14.720 G 14.750 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:56.04 +51:46:16.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:56.04 +51:46:16.2: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 16 56.04 +51 46 16.2 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991990683541947776,2461255.6577,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991990683541947776 20260803.1577 12.01CV 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 08 03.1577 2461255.6577 11.84 23:36:48.14 +54:33:55.2
112.16701 -6.73898 galactic Cas Second-epoch detections are separated by 1.0" and 3.2 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 1994315566520904064 | 23:36:44.27 +54:33:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:48.14 +54:33:55.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:48.14 +54:33:55.2: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 36 48.14 +54 33 55.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994315566520904064,2461255.6577,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994315566520904064 20260803.1577 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.95 23:21:05.72 +55:55:41.1
110.46334 -4.74113 galactic Cas Second-epoch detections are separated by 1.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:21:05.72 +55:55:41.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:05.72 +55:55:41.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:05.72 +55:55:41.1: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 21 05.72 +55 55 41.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.04 23:12:51.33 +55:43:33.6
109.30682 -4.51597 galactic Cas Second-epoch detections are separated by 2.0" and 3.2 pix
The object was found in VSX 3" Gaia DR3 1996778816166853888
Type: VAR
# Max. Min./Amp. JD0 Period
15.930 G 16.150 G 0.014757300000 F
ATTENTION: measured mag 12.04 is 3.9 mag brighter than the VSX record maximum brightness 15.93 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:51.33 +55:43:33.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:51.33 +55:43:33.6: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 12 51.33 +55 43 33.6 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996778816166853888,2461255.6577,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996778816166853888 20260803.1577 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.70 00:11:12.84 +57:36:28.0
117.54529 -4.84267 galactic Cas Second-epoch detections are separated by 2.1" 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 | ATO J002.8033+57.5971 | 00:11:12.84 +57:36:28.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:12.84 +57:36:28.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:11:12.84 +57:36:28.0: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 11 12.84 +57 36 28.0 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
ATO J002.8033+57.5971,2461255.6577,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.8033+57.5971 20260803.1577 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.76 23:35:48.19 +51:17:28.6
111.06295 -9.82909 galactic Cas Second-epoch detections are separated by 0.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.9516+51.2945 | 23:35:48.19 +51:17:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.669+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:48.19 +51:17:28.6: 13.62 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:35:48.19 +51:17:28.6: 13.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.62 +/- 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 08 03.1577* 23 35 48.19 +51 17 28.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.9516+51.2945,2461255.6577,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.9516+51.2945 20260803.1577 11.76CV 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 08 03.1577 2461255.6577 11.99 23:32:21.36 +53:10:40.3
111.12265 -7.87099 galactic Cas Second-epoch detections are separated by 0.8" 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 | ATO J353.0827+53.1779 | 23:32:21.36 +53:10:40.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.855+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:21.36 +53:10:40.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:32:21.36 +53:10:40.3: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 32 21.36 +53 10 40.3 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
ATO J353.0827+53.1779,2461255.6577,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.0827+53.1779 20260803.1577 11.99CV 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 08 03.1577 2461255.6577 11.96 23:29:15.19 +51:14:31.0
110.05773 -9.56382 galactic Cas Second-epoch detections are separated by 1.6" and 3.8 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 J352.3145+51.2458 | 23:29:15.19 +51:14:31.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.145+/-0.043 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:15.19 +51:14:31.0: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:29:15.19 +51:14:31.0: 13.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 29 15.19 +51 14 31.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.3145+51.2458,2461255.6577,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.3145+51.2458 20260803.1577 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.02 23:35:55.35 +53:26:18.6
111.71431 -7.78052 galactic Cas Second-epoch detections are separated by 1.8" and 3.3 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 1994008081222729600 | 23:35:58.46 +53:25:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.388+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:55.35 +53:26:18.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:35:55.35 +53:26:18.6: 13.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 35 55.35 +53 26 18.6 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994008081222729600,2461255.6577,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994008081222729600 20260803.1577 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 08 03.1577 2461255.6577 12.02 23:22:52.50 +51:52:56.4
109.32213 -8.63374 galactic And Second-epoch detections are separated by 3.3" and 3.0 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 1992319334439314432 | 23:22:51.40 +51:53:39.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.787+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:52.50 +51:52:56.4: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:52.50 +51:52:56.4: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 22 52.50 +51 52 56.4 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992319334439314432,2461255.6577,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992319334439314432 20260803.1577 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 08 03.1577 2461255.6577 12.12 23:10:01.96 +57:27:59.1
109.60348 -2.75748 galactic Cas Second-epoch detections are separated by 0.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J347.5124+57.4646 | 23:10:01.96 +57:27:59.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.292+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:01.96 +57:27:59.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:10:01.96 +57:27:59.1: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 10 01.96 +57 27 59.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5124+57.4646,2461255.6577,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5124+57.4646 20260803.1577 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 08 03.1577 2461255.6577 12.07 23:27:13.52 +56:44:18.1
111.53691 -4.25870 galactic Cas Second-epoch detections are separated by 1.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:13.52 +56:44:18.1 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.036 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:13.52 +56:44:18.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:13.52 +56:44:18.1: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 27 13.52 +56 44 18.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.26 23:21:16.89 +53:23:06.9
109.61091 -7.13862 galactic Cas Second-epoch detections are separated by 5.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1995695865928311680 | 23:21:15.11 +53:22:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:16.89 +53:23:06.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:16.89 +53:23:06.9: 13.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 21 16.89 +53 23 06.9 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995695865928311680,2461255.6577,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995695865928311680 20260803.1577 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.96 23:28:33.41 +49:24:17.0
109.35491 -11.26968 galactic And Second-epoch detections are separated by 2.8" 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 | 23:28:33.41 +49:24:17.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:33.41 +49:24:17.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:33.41 +49:24:17.0: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 28 33.41 +49 24 17.0 12.0 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,2461255.6577,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.10 23:20:51.80 +51:28:43.2
108.88564 -8.90594 galactic And Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:20:51.80 +51:28:43.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:51.80 +51:28:43.2: 13.32 +/- 0.26 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:51.80 +51:28:43.2: 13.48 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 08 03.1577* 23 20 51.80 +51 28 43.2 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,2461255.6577,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.85 00:07:17.65 +58:04:11.7
117.10478 -4.30152 galactic Cas Second-epoch detections are separated by 1.4" and 3.2 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 J001.8071+58.0668 | 00:07:13.54 +58:04:30.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1948PMcCO..10...57V BD+57 2869 J-Ks=0.350+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:17.65 +58:04:11.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:07:17.65 +58:04:11.7: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 07 17.65 +58 04 11.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.8071+58.0668,2461255.6577,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.8071+58.0668 20260803.1577 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 08 03.1577 2461255.6577 11.93 23:55:11.77 +54:35:56.4
114.77339 -7.37941 galactic Cas Second-epoch detections are separated by 1.7" 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 1993649571712577280 | 23:55:15.72 +54:35:48.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:11.77 +54:35:56.4: 12.86 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:55:11.77 +54:35:56.4: 12.94 +/- 0.18 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 55 11.77 +54 35 56.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993649571712577280,2461255.6577,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993649571712577280 20260803.1577 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.15 23:42:05.76 +53:06:25.4
112.51585 -8.35659 galactic Cas Second-epoch detections are separated by 2.5" and 3.7 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 | 23:42:05.76 +53:06:25.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:05.76 +53:06:25.4: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:42:05.76 +53:06:25.4: 13.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 42 05.76 +53 06 25.4 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
target,2461255.6577,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.20 23:14:39.05 +57:15:47.4
110.10584 -3.17854 galactic Cas Second-epoch detections are separated by 3.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.6460+57.2557 | 23:14:39.05 +57:15:47.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:39.05 +57:15:47.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:39.05 +57:15:47.4: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 14 39.05 +57 15 47.4 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 J348.6460+57.2557,2461255.6577,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.6460+57.2557 20260803.1577 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 11.88 00:10:04.69 +50:47:24.4
116.28160 -11.54680 galactic Cas Second-epoch detections are separated by 2.6" 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 | ATO J002.5137+50.7986 | 00:10:04.69 +50:47:24.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:04.69 +50:47:24.4: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:10:04.69 +50:47:24.4: 13.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 10 04.69 +50 47 24.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.5137+50.7986,2461255.6577,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.5137+50.7986 20260803.1577 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 08 03.1577 2461255.6577 12.05 23:53:22.56 +56:58:21.9
115.04996 -5.00781 galactic Cas Second-epoch detections are separated by 1.5" and 3.1 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 1998070055131912832 | 23:53:18.54 +56:57:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:22.56 +56:58:21.9: 12.96 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:53:22.56 +56:58:21.9: 13.08 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 08 03.1577* 23 53 22.56 +56 58 21.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998070055131912832,2461255.6577,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998070055131912832 20260803.1577 12.05CV 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 08 03.1577 2461255.6577 12.38 23:15:47.66 +56:18:48.4
109.90608 -4.12021 galactic Cas Second-epoch detections are separated by 1.6" and 2.9 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 J348.9555+56.3179 | 23:15:53.21 +56:18:45.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.641+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:47.66 +56:18:48.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:15:47.66 +56:18:48.4: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 15 47.66 +56 18 48.4 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.9555+56.3179,2461255.6577,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.9555+56.3179 20260803.1577 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.12 23:38:53.35 +51:52:36.4
111.69904 -9.40566 galactic Cas Second-epoch detections are separated by 0.7" and 3.7 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 1944845755243036288 | 23:38:53.60 +51:51:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:53.35 +51:52:36.4: 13.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:38:53.35 +51:52:36.4: 13.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 38 53.35 +51 52 36.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944845755243036288,2461255.6577,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944845755243036288 20260803.1577 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 08 03.1577 2461255.6577 12.37 23:26:58.61 +55:51:30.2
111.22053 -5.08096 galactic Cas Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:58.61 +55:51:30.2 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:58.61 +55:51:30.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:58.61 +55:51:30.2: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 26 58.61 +55 51 30.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.24 23:12:55.29 +55:44:24.2
109.32072 -4.50638 galactic Cas Second-epoch detections are separated by 0.2" and 3.1 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 1996778953605727232 | 23:12:59.93 +55:44:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.223+/-0.043 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:55.29 +55:44:24.2: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:55.29 +55:44:24.2: 13.43 +/- 0.31 detection
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 08 03.1577* 23 12 55.29 +55 44 24.2 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996778953605727232,2461255.6577,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996778953605727232 20260803.1577 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.02 23:44:00.08 +53:01:56.6
112.77490 -8.50430 galactic Cas Second-epoch detections are separated by 2.9" and 3.2 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 J355.9935+53.0252 | 23:44:00.08 +53:01:56.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:00.08 +53:01:56.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:44:00.08 +53:01:56.6: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 44 00.08 +53 01 56.6 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
ATO J355.9935+53.0252,2461255.6577,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.9935+53.0252 20260803.1577 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 08 03.1577 2461255.6577 12.11 23:24:41.12 +50:44:55.6
109.20555 -9.79637 galactic And Second-epoch detections are separated by 2.2" and 3.6 pix
The object was found in VSX22" Gaia DR3 1991268922877410688
Type: ROT
# Max. Min./Amp. JD0 Period
15.160 G 15.200 G G
ATTENTION: measured mag 12.11 is 3.1 mag brighter than the VSX record maximum brightness 15.16 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:41.12 +50:44:55.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:41.12 +50:44:55.6: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 24 41.12 +50 44 55.6 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991268922877410688,2461255.6577,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991268922877410688 20260803.1577 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.21 23:23:53.43 +49:30:41.6
108.66122 -10.91897 galactic And Second-epoch detections are separated by 2.6" 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 1943063000220602240 | 23:23:56.39 +49:31:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1958PMcCO..13b....V AG+49 2096 J-Ks=0.304+/-0.037 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:53.43 +49:30:41.6: 13.18 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:53.43 +49:30:41.6: 13.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.18 +/- 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 08 03.1577* 23 23 53.43 +49 30 41.6 12.2 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
Gaia DR3 1943063000220602240,2461255.6577,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943063000220602240 20260803.1577 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.29 23:28:42.69 +54:24:51.9
110.99351 -6.52854 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J352.1776+54.4142 | 23:28:42.69 +54:24:51.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.652+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:42.69 +54:24:51.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:42.69 +54:24:51.9: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 28 42.69 +54 24 51.9 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.1776+54.4142,2461255.6577,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.1776+54.4142 20260803.1577 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.32 23:15:33.52 +52:26:46.1
108.46180 -7.71105 galactic And Second-epoch detections are separated by 0.8" 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 | target | 23:15:33.52 +52:26:46.1 (user input) | T | P | (position from user input) J-Ks=0.892+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:33.52 +52:26:46.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:15:33.52 +52:26:46.1: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 15 33.52 +52 26 46.1 12.3 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,2461255.6577,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.46 23:21:40.71 +53:15:15.5
109.62175 -7.28196 galactic Cas Second-epoch detections are separated by 1.7" and 3.3 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 | ASASSN-V J232140.42+531439.1 | 23:21:40.42 +53:14:39.1 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:40.71 +53:15:15.5: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:40.71 +53:15:15.5: 13.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 21 40.71 +53 15 15.5 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J232140.42+531439.1,2461255.6577,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J232140.42+531439.1 20260803.1577 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.35 23:42:00.42 +54:28:43.7
112.87372 -7.03141 galactic Cas Second-epoch detections are separated by 0.6" and 3.3 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 1994216885352847872 | 23:41:56.03 +54:28:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.445+/-0.044 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:00.42 +54:28:43.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:42:00.42 +54:28:43.7: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 42 00.42 +54 28 43.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994216885352847872,2461255.6577,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994216885352847872 20260803.1577 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.20 23:53:41.06 +51:21:14.9
113.82011 -10.49297 galactic Cas Second-epoch detections are separated by 0.0" and 3.8 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 J358.4052+51.3477 | 23:53:40.47 +51:20:39.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:41.06 +51:21:14.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:53:41.06 +51:21:14.9: 13.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 53 41.06 +51 21 14.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.4052+51.3477,2461255.6577,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.4052+51.3477 20260803.1577 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.18 23:51:17.09 +57:27:59.2
114.88624 -4.46262 galactic Cas Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.8051+57.4585 | 23:51:17.83 +57:27:20.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.356+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:17.09 +57:27:59.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:51:17.09 +57:27:59.2: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 51 17.09 +57 27 59.2 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.8051+57.4585,2461255.6577,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.8051+57.4585 20260803.1577 12.18CV 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 08 03.1577 2461255.6577 12.52 23:17:09.56 +56:05:57.0
110.00650 -4.38837 galactic Cas Second-epoch detections are separated by 0.6" and 3.0 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 J349.2933+56.0937 | 23:17:10.26 +56:05:18.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.637+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:09.56 +56:05:57.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:09.56 +56:05:57.0: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 17 09.56 +56 05 57.0 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.2933+56.0937,2461255.6577,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.2933+56.0937 20260803.1577 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.39 23:24:47.36 +51:03:21.4
109.32513 -9.51225 galactic And Second-epoch detections are separated by 2.2" and 3.8 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 1991289332561816192 | 23:24:49.23 +51:02:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:47.36 +51:03:21.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:47.36 +51:03:21.4: 13.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 24 47.36 +51 03 21.4 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991289332561816192,2461255.6577,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991289332561816192 20260803.1577 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.71 23:10:21.25 +56:59:48.6
109.46459 -3.20822 galactic Cas Second-epoch detections are separated by 0.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J347.5891+57.0002 | 23:10:21.25 +56:59:48.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.466+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:21.25 +56:59:48.6: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:10:21.25 +56:59:48.6: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 10 21.25 +56 59 48.6 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5891+57.0002,2461255.6577,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5891+57.0002 20260803.1577 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.49 23:24:46.68 +52:18:02.5
109.74251 -8.33777 galactic And Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:46.68 +52:18:02.5 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.041 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:46.68 +52:18:02.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:46.68 +52:18:02.5: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 24 46.68 +52 18 02.5 12.5 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
target,2461255.6577,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.48 23:21:20.30 +49:31:45.4
108.27117 -10.76047 galactic And Second-epoch detections are separated by 1.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:21:20.30 +49:31:45.4 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:20.30 +49:31:45.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:20.30 +49:31:45.4: 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 08 03.1577* 23 21 20.30 +49 31 45.4 12.5 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
target,2461255.6577,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.46 23:30:41.74 +57:06:29.4
112.10411 -4.05643 galactic Cas Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:41.74 +57:06:29.4 (user input) | T | P | (position from user input) J-Ks=0.794+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:41.74 +57:06:29.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:41.74 +57:06:29.4: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 41.74 +57 06 29.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.59 23:22:49.28 +56:16:31.4
110.80882 -4.49627 galactic Cas Second-epoch detections are separated by 2.7" and 3.2 pix
The object was found in VSX22" Gaia DR3 1997220235721984512
Type: ROT
# Max. Min./Amp. JD0 Period
15.870 G 15.910 G K
ATTENTION: measured mag 12.59 is 3.3 mag brighter than the VSX record maximum brightness 15.87 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:49.28 +56:16:31.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:49.28 +56:16:31.4: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 22 49.28 +56 16 31.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997220235721984512,2461255.6577,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997220235721984512 20260803.1577 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.47 23:27:30.19 +54:55:09.7
110.98865 -5.99425 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 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 | 23:27:30.19 +54:55:09.7 (user input) | T | P | (position from user input) J-Ks=0.861+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:30.19 +54:55:09.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:30.19 +54:55:09.7: 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 08 03.1577* 23 27 30.19 +54 55 09.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.57 23:19:00.00 +52:31:08.7
108.98182 -7.83092 galactic And Second-epoch detections are separated by 3.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:19:00.00 +52:31:08.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:00.00 +52:31:08.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:00.00 +52:31:08.7: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 19 00.00 +52 31 08.7 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.41 23:24:44.80 +53:30:14.1
110.14079 -7.20109 galactic Cas Second-epoch detections are separated by 1.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:44.80 +53:30:14.1 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:44.80 +53:30:14.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:44.80 +53:30:14.1: 13.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 24 44.80 +53 30 14.1 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.59 23:11:37.88 +55:12:40.4
108.95195 -4.92829 galactic Cas Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J347.9014+55.2228 | 23:11:37.88 +55:12:40.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.841+/-0.049 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:37.88 +55:12:40.4: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:11:37.88 +55:12:40.4: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 11 37.88 +55 12 40.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.9014+55.2228,2461255.6577,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.9014+55.2228 20260803.1577 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.38 23:49:31.85 +52:38:02.7
113.49192 -9.09928 galactic Cas Second-epoch detections are separated by 2.5" and 3.2 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 | ASASSN-V J234935.80+523816.3 | 23:49:35.80 +52:38:16.3 (Gaia DR3) | SR (local) | 42.640000000000 (local) | Gaia3var=VARIABLE J-Ks=0.649+/-0.037 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:31.85 +52:38:02.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:49:31.85 +52:38:02.7: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 49 31.85 +52 38 02.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J234935.80+523816.3,2461255.6577,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J234935.80+523816.3 20260803.1577 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.51 23:26:36.90 +50:52:54.8
109.54211 -9.77138 galactic Cas Second-epoch detections are separated by 1.8" and 3.9 pix
The object was found in VSX 9" Gaia DR3 1991318916295917184
Type:
# Max. Min./Amp. JD0 Period
15.150 G 15.190 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:36.90 +50:52:54.8: 13.73 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:36.90 +50:52:54.8: 13.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.73 +/- 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 08 03.1577* 23 26 36.90 +50 52 54.8 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991318916295917184,2461255.6577,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991318916295917184 20260803.1577 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.53 23:34:40.85 +54:45:09.4
111.92628 -6.47065 galactic Cas Second-epoch detections are separated by 1.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.6767+54.7466 | 23:34:40.85 +54:45:09.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.493+/-0.043 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:40.85 +54:45:09.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:40.85 +54:45:09.4: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 34 40.85 +54 45 09.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.6767+54.7466,2461255.6577,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.6767+54.7466 20260803.1577 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.76 23:23:15.10 +53:50:12.7
110.04250 -6.81333 galactic Cas Second-epoch detections are separated by 2.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:23:15.10 +53:50:12.7 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:15.10 +53:50:12.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:15.10 +53:50:12.7: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 23 15.10 +53 50 12.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.68 23:18:37.91 +55:18:04.0
109.91725 -5.20814 galactic Cas Second-epoch detections are separated by 2.9" and 3.6 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 J349.6499+55.2967 | 23:18:37.91 +55:18:04.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.428+/-0.043 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:37.91 +55:18:04.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:37.91 +55:18:04.0: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 18 37.91 +55 18 04.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.6499+55.2967,2461255.6577,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.6499+55.2967 20260803.1577 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.63 23:33:53.96 +51:29:45.2
110.83665 -9.54571 galactic Cas Second-epoch detections are separated by 1.5" and 3.7 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 | 23:33:53.96 +51:29:45.2 (user input) | T | P | (position from user input) J-Ks=0.703+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:53.96 +51:29:45.2: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:33:53.96 +51:29:45.2: 13.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 33 53.96 +51 29 45.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.38 23:47:50.81 +51:54:48.6
113.06051 -9.73525 galactic Cas Second-epoch detections are separated by 0.5" and 3.8 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 1945071636168346368 | 23:47:51.64 +51:54:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:50.81 +51:54:48.6: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:50.81 +51:54:48.6: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 47 50.81 +51 54 48.6 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1945071636168346368,2461255.6577,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945071636168346368 20260803.1577 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.56 23:27:46.31 +56:30:45.6
111.53597 -4.49658 galactic Cas Second-epoch detections are separated by 2.4" and 3.2 pix
The object was found in VSX 0" Gaia DR3 1997063349158881152
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.200 G 14.220 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:46.31 +56:30:45.6: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:46.31 +56:30:45.6: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 27 46.31 +56 30 45.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997063349158881152,2461255.6577,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997063349158881152 20260803.1577 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.29 00:03:20.01 +57:13:23.6
116.43004 -5.04001 galactic Cas Second-epoch detections are separated by 1.5" and 3.2 pix
The object was found in VSX22" Gaia DR3 422567852144424320
Type: VAR
# Max. Min./Amp. JD0 Period
16.880 G 17.180 G 0.018203900000 K
ATTENTION: measured mag 12.29 is 4.6 mag brighter than the VSX record maximum brightness 16.88 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:20.01 +57:13:23.6: 13.63 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:03:20.01 +57:13:23.6: 13.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 03 20.01 +57 13 23.6 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 422567852144424320,2461255.6577,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422567852144424320 20260803.1577 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.48 23:30:12.31 +55:03:27.7
111.40232 -5.98527 galactic Cas Second-epoch detections are separated by 0.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:12.31 +55:03:27.7 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.034 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:12.31 +55:03:27.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:12.31 +55:03:27.7: 13.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 12.31 +55 03 27.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.55 23:19:35.87 +56:55:08.6
110.61177 -3.73964 galactic Cas Second-epoch detections are separated by 0.9" and 3.1 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 | 23:19:35.87 +56:55:08.6 (user input) | T | P | (position from user input) J-Ks=0.953+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:35.87 +56:55:08.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:35.87 +56:55:08.6: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 19 35.87 +56 55 08.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.68 23:30:08.69 +52:34:41.0
110.61537 -8.33880 galactic Cas Second-epoch detections are separated by 2.8" and 3.2 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 J352.5334+52.5665 | 23:30:08.69 +52:34:41.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.490+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:08.69 +52:34:41.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:08.69 +52:34:41.0: 13.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 08.69 +52 34 41.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.5334+52.5665,2461255.6577,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.5334+52.5665 20260803.1577 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.55 23:33:32.25 +55:22:41.6
111.95550 -5.82463 galactic Cas Second-epoch detections are separated by 0.9" 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 | ATO J353.3657+55.3740 | 23:33:32.25 +55:22:41.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.524+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:32.25 +55:22:41.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:33:32.25 +55:22:41.6: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 33 32.25 +55 22 41.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.3657+55.3740,2461255.6577,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.3657+55.3740 20260803.1577 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.71 23:19:08.81 +57:15:13.4
110.67115 -3.40462 galactic Cas Second-epoch detections are separated by 1.1" and 2.7 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 | 23:19:08.81 +57:15:13.4 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:08.81 +57:15:13.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:08.81 +57:15:13.4: 13.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 19 08.81 +57 15 13.4 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.45 23:47:13.67 +57:22:32.7
114.33261 -4.42003 galactic Cas Second-epoch detections are separated by 1.2" 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 | target | 23:47:13.67 +57:22:32.7 (user input) | T | P | (position from user input) J-Ks=0.985+/-0.034 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:13.67 +57:22:32.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:13.67 +57:22:32.7: 13.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 47 13.67 +57 22 32.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.46 23:46:36.09 +57:25:52.7
114.26447 -4.34529 galactic Cas Second-epoch detections are separated by 2.3" and 3.0 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 | 23:46:36.09 +57:25:52.7 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:36.09 +57:25:52.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:46:36.09 +57:25:52.7: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 46 36.09 +57 25 52.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.81 23:14:14.72 +52:54:28.7
108.44598 -7.20839 galactic And Second-epoch detections are separated by 2.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:14:14.72 +52:54:28.7 (user input) | T | P | (position from user input) J-Ks=0.720+/-0.037 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:14.72 +52:54:28.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:14.72 +52:54:28.7: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 14 14.72 +52 54 28.7 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.61 23:33:16.07 +53:01:37.5
111.20836 -8.05609 galactic Cas Second-epoch detections are separated by 1.8" and 3.3 pix
The object was found in VSX 1" Gaia DR3 1993227015649012480
Type: ROT
# Max. Min./Amp. JD0 Period
14.390 G 14.430 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:16.07 +53:01:37.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:33:16.07 +53:01:37.5: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 33 16.07 +53 01 37.5 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993227015649012480,2461255.6577,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993227015649012480 20260803.1577 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.61 23:22:00.76 +50:11:27.6
108.60737 -10.17704 galactic And Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:22:00.76 +50:11:27.6 (user input) | T | P | (position from user input) J-Ks=0.757+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:00.76 +50:11:27.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:00.76 +50:11:27.6: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 22 00.76 +50 11 27.6 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.71 23:25:07.58 +54:12:38.1
110.42916 -6.55260 galactic Cas Second-epoch detections are separated by 2.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:07.58 +54:12:38.1 (user input) | T | P | (position from user input) J-Ks=1.006+/-0.032 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:07.58 +54:12:38.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:07.58 +54:12:38.1: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 25 07.58 +54 12 38.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.71 23:39:19.81 +56:14:20.3
112.98715 -5.23416 galactic Cas Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:19.81 +56:14:20.3 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:19.81 +56:14:20.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:39:19.81 +56:14:20.3: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 39 19.81 +56 14 20.3 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.66 23:18:40.79 +52:55:57.3
109.08333 -7.42693 galactic And Second-epoch detections are separated by 2.2" 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 | target | 23:18:40.79 +52:55:57.3 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:40.79 +52:55:57.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:40.79 +52:55:57.3: 13.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 18 40.79 +52 55 57.3 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.64 23:30:55.38 +51:58:02.6
110.53756 -8.95619 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:55.38 +51:58:02.6 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.042 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:55.38 +51:58:02.6: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:55.38 +51:58:02.6: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 30 55.38 +51 58 02.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.59 23:24:22.90 +50:20:34.9
109.02158 -10.16261 galactic And Second-epoch detections are separated by 2.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:22.90 +50:20:34.9 (user input) | T | P | (position from user input) J-Ks=0.274+/-0.040 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:22.90 +50:20:34.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:22.90 +50:20:34.9: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 24 22.90 +50 20 34.9 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.79 23:25:33.09 +56:08:21.5
111.12281 -4.75060 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 23:25:33.09 +56:08:21.5 (user input) | T | P | (position from user input) J-Ks=0.259+/-0.038 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:33.09 +56:08:21.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:33.09 +56:08:21.5: 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 08 03.1577* 23 25 33.09 +56 08 21.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.63 23:41:42.44 +54:39:45.5
112.88121 -6.84266 galactic Cas Second-epoch detections are separated by 1.5" and 3.6 pix
The object was found in VSX 3" Gaia DR3 1994234374459560960
Type: ROT
# Max. Min./Amp. JD0 Period
15.110 G 15.160 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:42.44 +54:39:45.5: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:41:42.44 +54:39:45.5: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 41 42.44 +54 39 45.5 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994234374459560960,2461255.6577,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994234374459560960 20260803.1577 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.62 23:53:53.39 +55:17:53.2
114.74425 -6.65615 galactic Cas Second-epoch detections are separated by 0.6" 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 | target | 23:53:53.39 +55:17:53.2 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.040 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:53.39 +55:17:53.2: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:53:53.39 +55:17:53.2: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 53 53.39 +55 17 53.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.77 23:48:02.65 +56:26:08.5
114.20943 -5.35867 galactic Cas Second-epoch detections are separated by 3.4" and 2.9 pix
The object was found in VSX16" Gaia DR3 1997926946821730816
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.760 G 15.800 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:02.65 +56:26:08.5: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:48:02.65 +56:26:08.5: 13.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 48 02.65 +56 26 08.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997926946821730816,2461255.6577,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997926946821730816 20260803.1577 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.64 23:31:05.16 +55:00:38.8
111.50843 -6.06888 galactic Cas Second-epoch detections are separated by 0.8" and 3.1 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 | 23:31:05.16 +55:00:38.8 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.056 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:05.16 +55:00:38.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:05.16 +55:00:38.8: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 31 05.16 +55 00 38.8 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.60 23:36:47.01 +55:28:07.8
112.42485 -5.87259 galactic Cas Second-epoch detections are separated by 2.2" and 3.6 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 J354.2083+55.4779 | 23:36:47.01 +55:28:07.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.712+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:47.01 +55:28:07.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:47.01 +55:28:07.8: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 36 47.01 +55 28 07.8 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.2083+55.4779,2461255.6577,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.2083+55.4779 20260803.1577 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.71 23:47:25.88 +57:23:38.1
114.36376 -4.40918 galactic Cas Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:47:25.88 +57:23:38.1 (user input) | T | P | (position from user input) J-Ks=1.182+/-0.034 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:25.88 +57:23:38.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:25.88 +57:23:38.1: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 47 25.88 +57 23 38.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.68 00:01:50.67 +55:27:32.4
115.89068 -6.73329 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 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 420508466866496512 | 00:01:47.85 +55:27:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:50.67 +55:27:32.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:01:50.67 +55:27:32.4: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 00 01 50.67 +55 27 32.4 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420508466866496512,2461255.6577,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420508466866496512 20260803.1577 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.50 00:16:51.06 +57:09:34.2
118.23450 -5.39646 galactic Cas Second-epoch detections are separated by 1.6" and 3.8 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 | 00:16:51.06 +57:09:34.2 (user input) | T | P | (position from user input) J-Ks=1.254+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:16:51.06 +57:09:34.2: 13.64 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:16:51.06 +57:09:34.2: 13.76 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.64 +/- 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 08 03.1577* 00 16 51.06 +57 09 34.2 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.50CV 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 08 03.1577 2461255.6577 12.88 23:41:24.78 +55:36:49.5
113.09774 -5.91526 galactic Cas Second-epoch detections are separated by 0.9" and 3.1 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 | 23:41:24.78 +55:36:49.5 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:24.78 +55:36:49.5: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:41:24.78 +55:36:49.5: 13.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 41 24.78 +55 36 49.5 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.77 23:48:28.52 +56:23:56.5
114.25856 -5.40874 galactic Cas Second-epoch detections are separated by 2.3" and 3.2 pix
The object was found in VSX 1" Gaia DR3 1997949143213223552
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.530 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:28.52 +56:23:56.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:48:28.52 +56:23:56.5: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.1577* 23 48 28.52 +56 23 56.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997949143213223552,2461255.6577,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997949143213223552 20260803.1577 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.65 23:47:04.41 +51:55:58.8
112.94827 -9.68670 galactic Cas Second-epoch detections are separated by 3.3" and 3.6 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 | ASASSN-V J234709.10+515603.3 | 23:47:09.12 +51:56:03.3 (Gaia DR3) | L (local) | d (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.454+/-0.041 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:04.41 +51:55:58.8: 13.59 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:04.41 +51:55:58.8: 13.66 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 08 03.1577* 23 47 04.41 +51 55 58.8 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J234709.10+515603.3,2461255.6577,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J234709.10+515603.3 20260803.1577 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1577 2461255.6577 12.65 23:55:29.15 +54:30:22.2
114.79437 -7.47915 galactic Cas Second-epoch detections are separated by 1.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:55:29.15 +54:30:22.2 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.043 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:29.15 +54:30:22.2: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:55:29.15 +54:30:22.2: 13.91 +/- 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 08 03.1577* 23 55 29.15 +54 30 22.2 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461255.6577,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260803.1577 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461255.65793102 03.08.2026 03:47:15.240 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 17 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 20825
Objects passed selection criteria: 20803
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 19283
Average stars matched: 18882.8 (97.9243 %)
Memory usage VmPeak: 247164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 23:11:11 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: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461255.65793102 03.08.2026 03:47:15.240 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 478
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 310 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 162916
Objects passed selection criteria: 162507
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 151206
Average stars matched: 146118 (96.6355 %)
Memory usage VmPeak: 577032 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 23:18:01 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.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: 2461255.65741605
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits'
wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits'
wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 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: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
Image size: 938.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.885 +53:59:48.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.885 +53:59:48.85
Angular distance between the image centers 0.0255 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
Image size: 938.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.078 +53:59:34.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:01.078 +53:59:34.12
Angular distance between the image centers 0.0274 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:02.885 +53:59:48.85
Second-epoch second image center 00:00:01.078 +53:59:34.12
Angular distance between the image centers 0.00603 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.w8pEbMSex9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits &> /tmp/tmp.92t4CByQl0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits &> /tmp/tmp.2BYpn1zrxu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits &> /tmp/tmp.RdMZdJpE1F
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0821 to 14.9840 deg, Dec +48.2682 to +59.2677 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 345.0821 to 14.9840 deg, Dec 48.2682 to 59.2677 deg
Loaded 25149 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
ERROR: only 52 of 25149 matchable stars (28951 detected on the reference image) matched the Tycho-2 photometric calibration catalog (0.21%) - 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 22.575300
a=0.000000 b=1.000000 c=22.575300
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0821 to 14.9840 deg, Dec +48.2682 to +59.2677 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 345.0821 to 14.9840 deg, Dec 48.2682 to 59.2677 deg
Loaded 25149 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28570 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0823 to 14.9843 deg, Dec +48.2680 to +59.2686 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 345.0823 to 14.9843 deg, Dec 48.2680 to 59.2686 deg
Loaded 25151 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 62 total matches.
Matched with Tycho-2 62 out of 28570 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
14.6 mag. fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
14.6 mag. fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (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.w8pEbMSex9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (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 345.0821 through 0 to 14.9840, gap 14.9840 to 345.0821
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3491 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2179 matched stars entering correct_measured_positions(), 2402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2040 matched stars entering correct_measured_positions(), 23307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.92"
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 345.0820 through 0 to 15.0032, gap 15.0032 to 345.0820
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3563 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2451 matched stars entering correct_measured_positions(), 23308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.07"
Accuracy estimation diagnostic: 2380 matched stars entering correct_measured_positions(), 23397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.12"
Excluding outliers - 2380 stars left (next iteration limit 2244)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=2380 sigma_overall_arcsec=12.078 sigma_q1_arcsec=29.329 sigma_q2_arcsec=29.014 sigma_q3_arcsec=5.984 sigma_q4_arcsec=5.684 n_q1=514 n_q2=285 n_q3=882 n_q4=699 worst_quadrant_to_overall_ratio=2.428
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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.92t4CByQl0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2755, bad_region=6825, passed=28570
Got 28570 stars (including 19480 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat
util/solve_plate_with_UCAC5 got 28570 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (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 345.0823 through 0 to 14.9843, gap 14.9843 to 345.0823
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3497 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2173 matched stars entering correct_measured_positions(), 2402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2035 matched stars entering correct_measured_positions(), 22970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.99"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0792 through 0 to 15.0034, gap 15.0034 to 345.0792
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3582 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2451 matched stars entering correct_measured_positions(), 22971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.15"
Accuracy estimation diagnostic: 2378 matched stars entering correct_measured_positions(), 23037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.01"
Excluding outliers - 2378 stars left (next iteration limit 2238)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits N_match=2378 sigma_overall_arcsec=11.840 sigma_q1_arcsec=29.033 sigma_q2_arcsec=28.890 sigma_q3_arcsec=5.697 sigma_q4_arcsec=5.199 n_q1=506 n_q2=300 n_q3=879 n_q4=693 worst_quadrant_to_overall_ratio=2.452
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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.2BYpn1zrxu (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_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.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_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1607, bad_region=3963, passed=20829
Got 20829 stars (including 15468 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat
util/solve_plate_with_UCAC5 got 20829 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9387 through 0 to 14.8393, gap 14.8393 to 344.9387
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 17793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9382 through 0 to 14.8394, gap 14.8394 to 344.9382
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 17793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 17793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4910 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4910 robust_rms=5.892 arcsec worst_quadrant_rms=9.713 arcsec
SIP_REFIT: SIP order 3 trial: matched=4910 robust_rms=0.555 arcsec worst_quadrant_rms=0.634 arcsec
SIP_REFIT: SIP order 5 trial: matched=4910 robust_rms=0.499 arcsec worst_quadrant_rms=0.533 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4910 robust_rms_before=0.783 arcsec robust_rms_before_corrected=0.532 arcsec robust_rms_after=0.499 arcsec worst_quadrant_rms_before=0.570 worst_quadrant_rms_after=0.533
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.570 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits N_match=4910 sigma_overall_arcsec=0.527 sigma_q1_arcsec=0.505 sigma_q2_arcsec=0.515 sigma_q3_arcsec=0.577 sigma_q4_arcsec=0.549 n_q1=1549 n_q2=801 n_q3=1645 n_q4=915 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.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.RdMZdJpE1F (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_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.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_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1599, bad_region=3950, passed=20843
Got 20843 stars (including 15494 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat
util/solve_plate_with_UCAC5 got 20843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9280 through 0 to 14.8388, gap 14.8388 to 344.9280
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 17806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9276 through 0 to 14.8390, gap 14.8390 to 344.9276
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 17806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 17806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4902 stars left (next iteration limit 5393)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4902 robust_rms=5.929 arcsec worst_quadrant_rms=9.754 arcsec
SIP_REFIT: SIP order 3 trial: matched=4902 robust_rms=0.559 arcsec worst_quadrant_rms=0.627 arcsec
SIP_REFIT: SIP order 5 trial: matched=4902 robust_rms=0.504 arcsec worst_quadrant_rms=0.539 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4902 robust_rms_before=0.779 arcsec robust_rms_before_corrected=0.532 arcsec robust_rms_after=0.504 arcsec worst_quadrant_rms_before=0.583 worst_quadrant_rms_after=0.539
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.583 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits N_match=4902 sigma_overall_arcsec=0.548 sigma_q1_arcsec=0.526 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.589 sigma_q4_arcsec=0.566 n_q1=1551 n_q2=799 n_q3=1637 n_q4=915 worst_quadrant_to_overall_ratio=1.074
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits sigma_overall=12.078 worst_q_ratio=2.428
ref2=Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits sigma_overall=11.840 worst_q_ratio=2.452
new1=fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits sigma_overall=0.527 worst_q_ratio=1.094
new2=fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits sigma_overall=0.548 worst_q_ratio=1.074
reference average sigma_overall=11.959 worst_q_ratio=2.44
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (2380 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 11.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469_astrometric_residuals.png (2378 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 10.68 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082_astrometric_residuals.png (4910 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083_astrometric_residuals.png (4902 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-46-30_20.00sec_0.00C_LIGHT_0082.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Cas-04-Q2b1x1_225054_TTUQ2b1x1_4188619_SfqUEQHA/wcs_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:25.78 +55:34:09.6: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:40.44 +53:43:09.9: 15.11 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:41.71 +51:32:27.1: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:59.75 +56:24:09.8: 15.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:49.50 +54:16:21.0: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:52.55 +53:58:00.7: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:39.30 +51:19:02.0: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:13:49.50 +54:16:21.0: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:25.78 +55:34:09.6: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:41.71 +51:32:27.1: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:59.75 +56:24:09.8: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:39.30 +51:19:02.0: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:54:40.44 +53:43:09.9: 15.55 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.11 +/- 0.24
Forced photometry filter KEPT candidate at 23:54:40.44 +53:43:09.9: ref_mag=15.11 +/- 0.24 new_mean_mag=11.6205 delta=3.49 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:53:52.55 +53:58:00.7: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:29.90 +50:16:46.5: 14.78 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:34.10 +51:01:38.9: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:03.42 +54:31:56.1: 14.74 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:29.90 +50:16:46.5: 15.14 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.16
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:30:34.10 +51:01:38.9: 15.57 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 23:21:29.90 +50:16:46.5: ref_mag=14.91 +/- 0.16 new_mean_mag=11.9727 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:03.42 +54:31:56.1: 14.99 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.14
Forced photometry filter KEPT candidate at 23:22:03.42 +54:31:56.1: ref_mag=14.83 +/- 0.14 new_mean_mag=12.0224 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:03.83 +53:01:45.7: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:58:03.83 +53:01:45.7: 15.55 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out31310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31459.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31310_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31310_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:53:52.55 +53:58:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.536 1993567658094807296 358.46887860052 +53.96700228800 11.7415 10.9240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31313_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31313_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:31:39.30 +51:19:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.233 1991345716892833408 352.91336519536 +51.31697839220 11.5913 10.7313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31315_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31315_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:20:41.71 +51:32:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.357 1992289407106736000 350.17415436338 +51.54116313948 12.1083 11.7507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31318_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31318_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:36:32.42 +52:37:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31397_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31397_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:11.87 +50:00:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31402_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31402_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:14:59.75 +56:24:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 3.515 2009196734847729792 348.74722010902 +56.40288939213 11.1735 10.2706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31413_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31413_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:54:40.44 +53:43:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.438 1945515765845536384 358.66833016645 +53.71980337108 11.5755 11.1605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31415_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31415_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:20:22.36 +54:45:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31428_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31428_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:30:25.78 +55:34:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.949 1997652927908347776 352.60703591407 +55.56948527992 11.6251 10.7944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31431_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31431_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:13:49.50 +54:16:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.362 1996407009436474496 348.45641030201 +54.27246302900 11.8015 11.6654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31441_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31441_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:29.90 +50:16:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.475 1991186047188063104 350.37437864068 +50.27956591572 11.8142 11.1132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31444_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31444_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:15:50.60 +57:32:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31447_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31447_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:09:14.28 +55:08:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31448_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31448_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:22:03.42 +54:31:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.874 1996003690523145728 350.51462517909 +54.53301812335 12.0525 11.2487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31449_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31449_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:30:34.10 +51:01:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.611 1943294309978851712 352.64183109914 +51.02741175906 11.7926 11.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31459_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31459_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:58:03.83 +53:01:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.897 1945241613793508480 359.51564392092 +53.02886913080 12.1298 11.6600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31464_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 31464_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:25.82 +52:02:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 07077_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:09:36.48 +51:34:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 21482_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:31.82 +56:34:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 06239_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 226964_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226964_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226966_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226966_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226981_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 226981_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227027_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227027_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227039_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227039_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227040_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227040_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227041_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227041_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227045_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227045_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227052_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227052_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227056_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227056_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 227058_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227058_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227059_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227059_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227063_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227063_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227069_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227069_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227074_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227074_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227075_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227075_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227079_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227079_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227081_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227081_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227097_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227097_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227099_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227099_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227101_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227101_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227103_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227103_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227110_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227110_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227118_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227118_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227119_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227119_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227120_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227120_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227123_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227123_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227126_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227126_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227127_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227127_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227131_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227131_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227137_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227137_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227145_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227145_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227147_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227147_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227169_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227169_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227170_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227170_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227176_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227176_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227179_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227179_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227186_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227186_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227192_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227192_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:46.51 +54:01:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227193_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227193_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227196_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227196_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227197_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227197_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227214_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227214_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227215_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227215_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227223_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227223_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227225_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227225_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227230_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227230_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227231_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227231_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227247_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227247_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227248_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227248_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227250_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227250_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227252_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227252_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227253_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227253_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:37:32.50 +52:48:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227256_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227256_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227263_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227263_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227266_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227266_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 227268_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227268_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227270_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227270_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227272_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227272_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227283_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227283_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227287_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227287_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227288_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227288_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:58:35.18 +54:07:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227295_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227295_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227296_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227296_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227297_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227297_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227298_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227298_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227300_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227300_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227301_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227301_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227307_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227307_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227312_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227312_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:08:33.36 +56:46:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227313_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227313_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227318_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227318_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227329_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227329_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227333_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227333_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227335_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227335_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227337_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227337_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227340_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227340_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227341_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227341_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227345_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227345_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227346_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227346_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227350_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227350_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227352_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227352_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227354_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227354_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227359_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227359_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227366_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227366_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:37:13.88 +50:24:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227372_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227372_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:22:17.97 +54:20:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227373_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227373_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:29:32.79 +53:51:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227375_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227375_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:34:43.32 +51:31:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227382_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227382_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227385_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227385_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227401_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227401_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227404_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227404_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:54:48.15 +56:48:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227413_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227413_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:12:59.85 +54:44:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227415_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227415_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:27:43.12 +53:58:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227418_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227418_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227419_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227419_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227423_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227423_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227425_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227425_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227430_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227430_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227436_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227436_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227440_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227440_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227441_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227441_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:39.73 +50:04:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227444_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227444_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227446_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227446_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:04:21.76 +51:49:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227447_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227447_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227448_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227448_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227450_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227450_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227464_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227464_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227473_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227473_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227474_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227474_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227475_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227475_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227476_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227476_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227477_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227477_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227483_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227483_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227489_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227489_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227493_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227493_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227500_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227500_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227502_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227502_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227503_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227503_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227504_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227504_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227506_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227506_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227507_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227507_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227508_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227508_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227510_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227510_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227512_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227512_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227514_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227514_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227515_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227515_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227516_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227516_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227519_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227519_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:51:56.94 +54:36:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227527_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227527_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:59.06 +57:58:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227528_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227528_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227529_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227529_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227532_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227532_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227533_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227533_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227535_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227535_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227538_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227538_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227540_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227540_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227541_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227541_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227542_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227542_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227544_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227544_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227545_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227545_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:21:54.19 +51:47:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227547_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227547_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:39:37.60 +57:08:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227549_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227549_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227550_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227550_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227553_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227553_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227615_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227615_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227652_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227652_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227720_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227720_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 227723_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227723_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:11.17 +56:38:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227745_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227745_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 227762_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227762_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227779_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227779_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:43:12.98 +51:57:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227786_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227786_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227797_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227797_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 227805_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227805_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:43:56.57 +56:20:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227812_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227812_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227814_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227814_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227824_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227824_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:35.12 +50:17:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227834_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227834_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227906_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227906_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227915_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227915_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 227922_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227922_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227933_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227933_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227940_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227940_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:32:37.68 +54:45:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227955_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227955_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227960_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227960_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:23:25.71 +55:49:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227968_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227968_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:59.50 +50:26:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227971_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227971_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227973_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227973_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227976_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227976_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 227978_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227978_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 227985_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227985_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 227987_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 227987_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:31:43.86 +55:25:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228005_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228005_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:56:31.90 +53:44:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228009_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228009_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:18:17.36 +58:11:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228017_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228017_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228026_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228026_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228028_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228028_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:58:51.60 +54:42:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228045_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228045_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:36:00.75 +53:25:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228061_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228061_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:18:03.79 +49:50:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228064_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228064_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:13:03.00 +49:56:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228072_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228072_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:27:11.40 +53:53:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228074_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228074_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:20:12.22 +50:06:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228075_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228075_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228087_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228087_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228101_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228101_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228109_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228109_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:52:01.74 +50:05:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228110_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228110_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228120_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228120_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:29:41.04 +56:48:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228122_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228122_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228140_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228140_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:08:17.70 +52:45:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228142_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228142_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:32:35.00 +54:04:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228157_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228157_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:59:00.48 +53:16:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228158_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228158_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:47:36.75 +55:14:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228159_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228159_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228173_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228173_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228182_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228182_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228187_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228187_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:45:33.04 +52:22:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228189_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228189_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228197_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228197_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:51:04.18 +51:22:57.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228209_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228209_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228214_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228214_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228222_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228222_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:53:42.83 +56:31:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228223_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228223_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:47:01.84 +57:25:00.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 228237_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228237_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228244_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228244_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228249_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228249_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:12:36.39 +57:12:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228251_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228251_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:11:49.37 +54:49:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228264_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228264_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:12:07.18 +53:36:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228269_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228269_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:43:13.66 +53:08:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228280_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228280_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228290_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228290_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228293_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228293_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228302_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228302_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228304_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228304_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:20:15.53 +57:50:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228312_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228312_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228317_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228317_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:49.09 +50:34:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228319_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228319_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:19:48.80 +50:46:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228321_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228321_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:50:23.47 +54:12:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228322_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228322_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228329_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228329_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:36:14.94 +49:55:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228340_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228340_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228347_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228347_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:00:23.15 +56:50:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228353_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228353_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:55:07.04 +56:11:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228362_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228362_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228378_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228378_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:01:30.98 +53:51:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228381_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228381_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228387_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228387_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228398_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228398_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228400_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228400_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228401_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228401_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228406_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228406_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228411_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228411_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:34:47.84 +50:18:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228414_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228414_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228418_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228418_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228428_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228428_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228433_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228433_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:00:57.48 +53:16:22.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228435_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228435_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228444_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228444_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228448_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228448_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228453_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228453_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:21.90 +54:05:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228462_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228462_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228470_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228470_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 228473_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228473_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:27:17.01 +54:46:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228483_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228483_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:07:40.60 +57:11:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228484_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228484_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228486_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228486_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:51:28.13 +51:30:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228496_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228496_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228499_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228499_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228501_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228501_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228502_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228502_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228509_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228509_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:50:18.50 +50:02:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228520_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228520_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228523_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228523_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:44.67 +55:46:33.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 228530_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228530_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228543_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228543_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228545_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228545_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228553_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228553_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228555_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228555_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228561_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228561_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228571_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228571_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:38:09.09 +57:45:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228573_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228573_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228576_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228576_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228584_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228584_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:42.98 +53:44:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228585_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228585_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228591_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228591_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 228608_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228608_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228612_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228612_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:03:28.49 +55:39:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228637_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228637_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228642_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228642_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228658_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228658_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:42:56.35 +52:44:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228674_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228674_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228675_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228675_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228677_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228677_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228687_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228687_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:46:33.31 +55:12:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228692_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228692_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228700_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228700_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228717_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228717_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228730_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228730_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228740_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228740_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228745_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228745_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228750_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228750_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:11:11.11 +53:26:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228756_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228756_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228759_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228759_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228760_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228760_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 228774_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228774_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228776_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228776_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228798_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228798_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228801_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228801_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228803_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228803_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228809_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228809_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228811_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228811_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228825_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228825_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228826_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228826_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228841_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228841_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228843_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228843_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228852_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228852_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228856_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228856_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228857_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228857_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228861_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228861_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228868_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228868_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228880_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228880_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228889_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228889_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228890_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228890_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228901_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228901_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228904_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228904_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228914_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228914_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 228921_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228921_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228929_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228929_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228930_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 228930_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 228939_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228939_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228951_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228951_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228964_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228964_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228971_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228971_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228980_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228980_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228981_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228981_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228990_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228990_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228998_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228998_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 228999_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 228999_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229001_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229001_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229008_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229008_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229012_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229012_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229019_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229019_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229029_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229029_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229034_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229034_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229057_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229057_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229058_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229058_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229099_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229099_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229128_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229128_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229139_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229139_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229153_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229153_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229175_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229175_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 229179_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229179_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229185_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229185_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229237_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229237_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229244_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229244_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229247_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229247_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229248_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229248_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229250_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229250_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229276_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229276_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229296_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229296_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229311_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229311_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 229336_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 229336_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 229344_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 229344_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 121532_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 121532_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:20:22.45 +54:45:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216461_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 216461_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 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 215248_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 215248_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:33:19.14 +52:53:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191364_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 191364_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:59:54.23 +56:58:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54745_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 54745_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:25.78 +52:02:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 179100_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:15:50.54 +57:32:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 197606_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:31.83 +56:34:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 46841_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:09:36.49 +51:34:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083
The candidate 25587_fd_Cas-04-Q2b1x1_2026-08-02_22-47-15_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:11.84 +50:00:13.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 16s
make_report_in_HTML.sh TOTAL: 522s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:46:50.97 +51:56:32.5
00:13:43.99 +54:31:40.9
23:56:31.16 +56:29:02.3
00:05:12.25 +51:03:42.6
23:43:27.49 +50:48:57.4
23:25:06.28 +54:08:56.6
23:31:29.79 +51:07:11.3
23:44:15.73 +54:03:03.6
23:36:02.75 +51:05:47.2
00:09:51.69 +55:21:40.4
23:44:35.93 +58:00:16.5
23:23:05.57 +54:06:19.4
23:19:48.01 +49:13:46.3
23:37:19.82 +57:11:47.8
23:33:42.96 +53:40:49.7
23:21:44.29 +53:21:19.0
23:43:01.12 +51:44:15.3
23:30:19.86 +51:32:15.6
23:45:40.11 +49:42:46.8
23:26:34.69 +52:38:37.3
23:32:48.72 +55:10:10.9
23:18:56.86 +52:58:26.6
00:04:18.17 +51:52:27.3
23:41:04.22 +54:08:50.8
23:14:21.20 +52:49:14.4
23:49:10.71 +51:58:44.7
23:43:00.68 +55:31:09.9
23:43:58.95 +55:38:50.8
00:26:38.45 +56:47:19.5
23:23:49.35 +54:57:28.0
23:34:26.31 +55:43:52.0
00:10:25.94 +58:05:06.9
23:14:57.96 +55:18:41.3
23:20:01.49 +56:18:40.6
23:40:38.95 +54:06:04.1
23:42:32.90 +58:08:11.3
23:27:20.61 +49:42:14.3
23:36:53.88 +55:39:27.7
23:44:34.08 +53:02:55.9
23:30:56.68 +51:10:37.0
23:33:59.07 +52:15:29.4
00:16:04.69 +54:40:19.5
23:46:23.31 +57:38:21.1
23:08:56.46 +57:15:29.7
23:15:24.67 +54:15:49.6
23:14:20.68 +56:26:27.3
00:00:15.41 +57:43:09.0
23:26:03.13 +52:03:35.9
23:45:47.83 +57:16:15.9
23:31:09.82 +52:06:27.4
23:16:41.18 +54:20:20.5
23:36:46.48 +53:03:10.3
23:51:14.19 +53:29:30.8
23:24:22.77 +57:21:09.2
23:10:31.41 +57:14:50.0
23:48:45.32 +54:05:07.7
23:16:25.73 +52:40:53.5
23:19:42.05 +51:36:25.9
00:32:19.53 +57:14:54.2
23:32:25.57 +51:54:36.9
23:16:35.53 +55:47:09.3
23:12:31.74 +56:42:50.5
23:45:04.37 +55:00:31.4
23:27:29.39 +55:44:25.2
00:11:49.65 +56:14:26.5
23:49:44.61 +55:38:29.7
23:41:51.68 +54:39:58.9
23:35:14.12 +56:30:57.6
23:25:47.99 +52:39:36.7
23:22:39.83 +57:01:55.9
23:46:34.36 +57:42:58.1
23:15:55.87 +53:32:18.6
00:18:51.07 +50:04:25.7
23:17:56.22 +50:57:32.0
23:22:04.88 +53:49:28.0
23:25:02.89 +56:51:11.0
23:12:15.38 +56:31:13.1
23:22:30.80 +52:04:54.8
23:30:34.79 +51:52:37.3
23:27:54.70 +55:41:49.2
23:19:17.20 +52:37:40.5
23:19:35.45 +54:16:30.4
23:40:37.12 +56:24:23.9
23:17:17.48 +55:08:01.9
23:37:42.13 +52:46:09.3
23:23:04.22 +52:29:55.9
23:13:33.87 +53:34:52.7
23:16:55.84 +55:40:34.4
23:39:41.70 +57:16:05.3
23:29:51.32 +56:20:02.2
23:18:41.24 +54:16:19.5
23:46:43.16 +50:45:04.7
23:28:05.73 +55:31:17.7
23:20:50.24 +57:13:06.3
23:12:44.76 +54:33:22.2
23:17:35.31 +54:08:15.4
23:56:33.04 +56:44:30.9
23:12:41.15 +54:49:13.2
23:18:56.50 +53:20:37.9
23:37:54.62 +52:32:03.2
23:21:14.39 +55:23:14.2
23:11:10.96 +55:59:33.2
23:38:08.00 +53:36:18.4
23:19:15.91 +51:56:02.6
23:50:25.76 +49:51:14.2
23:31:12.57 +53:30:57.7
23:31:08.95 +54:16:09.2
23:36:32.69 +50:40:34.5
23:23:09.38 +56:38:52.8
23:15:52.45 +52:57:57.3
23:21:37.62 +55:42:58.8
23:26:05.79 +53:11:06.1
23:27:06.61 +56:40:02.3
23:26:19.35 +51:13:14.5
23:19:40.15 +50:08:15.6
23:22:36.51 +57:23:01.3
23:25:41.45 +55:09:05.3
23:13:38.70 +53:34:21.6
23:29:11.90 +53:11:19.2
23:28:27.08 +51:42:39.1
23:58:05.32 +56:28:01.7
23:16:50.72 +52:05:37.3
23:34:22.93 +53:50:20.2
23:23:47.56 +54:34:21.7
23:31:35.90 +53:08:29.6
23:25:28.04 +49:20:13.5
23:43:15.02 +51:40:39.5
23:16:38.05 +55:10:33.8
23:30:32.18 +49:52:18.7
23:50:05.36 +50:49:19.3
23:26:00.27 +52:50:48.1
23:29:24.24 +51:40:00.7
23:34:39.79 +51:08:28.0
23:33:10.17 +56:17:31.8
23:11:51.57 +55:18:28.9
23:24:46.31 +54:53:45.7
23:17:29.43 +52:31:58.8
23:16:56.04 +51:46:16.2
23:36:48.14 +54:33:55.2
23:21:05.72 +55:55:41.1
23:12:51.33 +55:43:33.6
00:11:12.84 +57:36:28.0
23:35:48.19 +51:17:28.6
23:32:21.36 +53:10:40.3
23:29:15.19 +51:14:31.0
23:35:55.35 +53:26:18.6
23:22:52.50 +51:52:56.4
23:10:01.96 +57:27:59.1
23:27:13.52 +56:44:18.1
23:21:16.89 +53:23:06.9
23:28:33.41 +49:24:17.0
23:20:51.80 +51:28:43.2
00:07:17.65 +58:04:11.7
23:55:11.77 +54:35:56.4
23:42:05.76 +53:06:25.4
23:14:39.05 +57:15:47.4
00:10:04.69 +50:47:24.4
23:53:22.56 +56:58:21.9
23:15:47.66 +56:18:48.4
23:38:53.35 +51:52:36.4
23:26:58.61 +55:51:30.2
23:12:55.29 +55:44:24.2
23:44:00.08 +53:01:56.6
23:24:41.12 +50:44:55.6
23:23:53.43 +49:30:41.6
23:28:42.69 +54:24:51.9
23:15:33.52 +52:26:46.1
23:21:40.71 +53:15:15.5
23:42:00.42 +54:28:43.7
23:53:41.06 +51:21:14.9
23:51:17.09 +57:27:59.2
23:17:09.56 +56:05:57.0
23:24:47.36 +51:03:21.4
23:10:21.25 +56:59:48.6
23:24:46.68 +52:18:02.5
23:21:20.30 +49:31:45.4
23:30:41.74 +57:06:29.4
23:22:49.28 +56:16:31.4
23:27:30.19 +54:55:09.7
23:19:00.00 +52:31:08.7
23:24:44.80 +53:30:14.1
23:11:37.88 +55:12:40.4
23:49:31.85 +52:38:02.7
23:26:36.90 +50:52:54.8
23:34:40.85 +54:45:09.4
23:23:15.10 +53:50:12.7
23:18:37.91 +55:18:04.0
23:33:53.96 +51:29:45.2
23:47:50.81 +51:54:48.6
23:27:46.31 +56:30:45.6
00:03:20.01 +57:13:23.6
23:30:12.31 +55:03:27.7
23:19:35.87 +56:55:08.6
23:30:08.69 +52:34:41.0
23:33:32.25 +55:22:41.6
23:19:08.81 +57:15:13.4
23:47:13.67 +57:22:32.7
23:46:36.09 +57:25:52.7
23:14:14.72 +52:54:28.7
23:33:16.07 +53:01:37.5
23:22:00.76 +50:11:27.6
23:25:07.58 +54:12:38.1
23:39:19.81 +56:14:20.3
23:18:40.79 +52:55:57.3
23:30:55.38 +51:58:02.6
23:24:22.90 +50:20:34.9
23:25:33.09 +56:08:21.5
23:41:42.44 +54:39:45.5
23:53:53.39 +55:17:53.2
23:48:02.65 +56:26:08.5
23:31:05.16 +55:00:38.8
23:36:47.01 +55:28:07.8
23:47:25.88 +57:23:38.1
00:01:50.67 +55:27:32.4
00:16:51.06 +57:09:34.2
23:41:24.78 +55:36:49.5
23:48:28.52 +56:23:56.5
23:47:04.41 +51:55:58.8
23:55:29.15 +54:30:22.2
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:46:50.97 +51:56:32.5
00:13:43.99 +54:31:40.9
23:56:31.16 +56:29:02.3
00:05:12.25 +51:03:42.6
23:43:27.49 +50:48:57.4
23:25:06.28 +54:08:56.6
23:31:29.79 +51:07:11.3
23:44:15.73 +54:03:03.6
23:36:02.75 +51:05:47.2
00:09:51.69 +55:21:40.4
23:44:35.93 +58:00:16.5
23:23:05.57 +54:06:19.4
23:19:48.01 +49:13:46.3
23:37:19.82 +57:11:47.8
23:33:42.96 +53:40:49.7
23:21:44.29 +53:21:19.0
23:43:01.12 +51:44:15.3
23:30:19.86 +51:32:15.6
23:45:40.11 +49:42:46.8
23:26:34.69 +52:38:37.3
23:32:48.72 +55:10:10.9
23:18:56.86 +52:58:26.6
00:04:18.17 +51:52:27.3
23:41:04.22 +54:08:50.8
23:14:21.20 +52:49:14.4
23:49:10.71 +51:58:44.7
23:43:00.68 +55:31:09.9
23:43:58.95 +55:38:50.8
00:26:38.45 +56:47:19.5
23:23:49.35 +54:57:28.0
23:34:26.31 +55:43:52.0
00:10:25.94 +58:05:06.9
23:14:57.96 +55:18:41.3
23:20:01.49 +56:18:40.6
23:40:38.95 +54:06:04.1
23:42:32.90 +58:08:11.3
23:27:20.61 +49:42:14.3
23:36:53.88 +55:39:27.7
23:44:34.08 +53:02:55.9
23:30:56.68 +51:10:37.0
23:33:59.07 +52:15:29.4
00:16:04.69 +54:40:19.5
23:46:23.31 +57:38:21.1
23:08:56.46 +57:15:29.7
23:15:24.67 +54:15:49.6
23:14:20.68 +56:26:27.3
00:00:15.41 +57:43:09.0
23:26:03.13 +52:03:35.9
23:45:47.83 +57:16:15.9
23:31:09.82 +52:06:27.4
23:16:41.18 +54:20:20.5
23:36:46.48 +53:03:10.3
23:51:14.19 +53:29:30.8
23:24:22.77 +57:21:09.2
23:10:31.41 +57:14:50.0
23:48:45.32 +54:05:07.7
23:16:25.73 +52:40:53.5
23:19:42.05 +51:36:25.9
00:32:19.53 +57:14:54.2
23:32:25.57 +51:54:36.9
23:16:35.53 +55:47:09.3
23:12:31.74 +56:42:50.5
23:45:04.37 +55:00:31.4
23:27:29.39 +55:44:25.2
00:11:49.65 +56:14:26.5
23:49:44.61 +55:38:29.7
23:41:51.68 +54:39:58.9
23:35:14.12 +56:30:57.6
23:25:47.99 +52:39:36.7
23:22:39.83 +57:01:55.9
23:46:34.36 +57:42:58.1
23:15:55.87 +53:32:18.6
00:18:51.07 +50:04:25.7
23:17:56.22 +50:57:32.0
23:22:04.88 +53:49:28.0
23:25:02.89 +56:51:11.0
23:12:15.38 +56:31:13.1
23:22:30.80 +52:04:54.8
23:30:34.79 +51:52:37.3
23:27:54.70 +55:41:49.2
23:19:17.20 +52:37:40.5
23:19:35.45 +54:16:30.4
23:40:37.12 +56:24:23.9
23:17:17.48 +55:08:01.9
23:37:42.13 +52:46:09.3
23:23:04.22 +52:29:55.9
23:13:33.87 +53:34:52.7
23:16:55.84 +55:40:34.4
23:39:41.70 +57:16:05.3
23:29:51.32 +56:20:02.2
23:18:41.24 +54:16:19.5
23:46:43.16 +50:45:04.7
23:28:05.73 +55:31:17.7
23:20:50.24 +57:13:06.3
23:12:44.76 +54:33:22.2
23:17:35.31 +54:08:15.4
23:56:33.04 +56:44:30.9
23:12:41.15 +54:49:13.2
23:18:56.50 +53:20:37.9
23:37:54.62 +52:32:03.2
23:21:14.39 +55:23:14.2
23:11:10.96 +55:59:33.2
23:38:08.00 +53:36:18.4
23:19:15.91 +51:56:02.6
23:50:25.76 +49:51:14.2
23:31:12.57 +53:30:57.7
23:31:08.95 +54:16:09.2
23:36:32.69 +50:40:34.5
23:23:09.38 +56:38:52.8
23:15:52.45 +52:57:57.3
23:21:37.62 +55:42:58.8
23:26:05.79 +53:11:06.1
23:27:06.61 +56:40:02.3
23:26:19.35 +51:13:14.5
23:19:40.15 +50:08:15.6
23:22:36.51 +57:23:01.3
23:25:41.45 +55:09:05.3
23:13:38.70 +53:34:21.6
23:29:11.90 +53:11:19.2
23:28:27.08 +51:42:39.1
23:58:05.32 +56:28:01.7
23:16:50.72 +52:05:37.3
23:34:22.93 +53:50:20.2
23:23:47.56 +54:34:21.7
23:31:35.90 +53:08:29.6
23:25:28.04 +49:20:13.5
23:43:15.02 +51:40:39.5
23:16:38.05 +55:10:33.8
23:30:32.18 +49:52:18.7
23:50:05.36 +50:49:19.3
23:26:00.27 +52:50:48.1
23:29:24.24 +51:40:00.7
23:34:39.79 +51:08:28.0
23:33:10.17 +56:17:31.8
23:11:51.57 +55:18:28.9
23:24:46.31 +54:53:45.7
23:17:29.43 +52:31:58.8
23:16:56.04 +51:46:16.2
23:36:48.14 +54:33:55.2
23:21:05.72 +55:55:41.1
23:12:51.33 +55:43:33.6
00:11:12.84 +57:36:28.0
23:35:48.19 +51:17:28.6
23:32:21.36 +53:10:40.3
23:29:15.19 +51:14:31.0
23:35:55.35 +53:26:18.6
23:22:52.50 +51:52:56.4
23:10:01.96 +57:27:59.1
23:27:13.52 +56:44:18.1
23:21:16.89 +53:23:06.9
23:28:33.41 +49:24:17.0
23:20:51.80 +51:28:43.2
00:07:17.65 +58:04:11.7
23:55:11.77 +54:35:56.4
23:42:05.76 +53:06:25.4
23:14:39.05 +57:15:47.4
00:10:04.69 +50:47:24.4
23:53:22.56 +56:58:21.9
23:15:47.66 +56:18:48.4
23:38:53.35 +51:52:36.4
23:26:58.61 +55:51:30.2
23:12:55.29 +55:44:24.2
23:44:00.08 +53:01:56.6
23:24:41.12 +50:44:55.6
23:23:53.43 +49:30:41.6
23:28:42.69 +54:24:51.9
23:15:33.52 +52:26:46.1
23:21:40.71 +53:15:15.5
23:42:00.42 +54:28:43.7
23:53:41.06 +51:21:14.9
23:51:17.09 +57:27:59.2
23:17:09.56 +56:05:57.0
23:24:47.36 +51:03:21.4
23:10:21.25 +56:59:48.6
23:24:46.68 +52:18:02.5
23:21:20.30 +49:31:45.4
23:30:41.74 +57:06:29.4
23:22:49.28 +56:16:31.4
23:27:30.19 +54:55:09.7
23:19:00.00 +52:31:08.7
23:24:44.80 +53:30:14.1
23:11:37.88 +55:12:40.4
23:49:31.85 +52:38:02.7
23:26:36.90 +50:52:54.8
23:34:40.85 +54:45:09.4
23:23:15.10 +53:50:12.7
23:18:37.91 +55:18:04.0
23:33:53.96 +51:29:45.2
23:47:50.81 +51:54:48.6
23:27:46.31 +56:30:45.6
00:03:20.01 +57:13:23.6
23:30:12.31 +55:03:27.7
23:19:35.87 +56:55:08.6
23:30:08.69 +52:34:41.0
23:33:32.25 +55:22:41.6
23:19:08.81 +57:15:13.4
23:47:13.67 +57:22:32.7
23:46:36.09 +57:25:52.7
23:14:14.72 +52:54:28.7
23:33:16.07 +53:01:37.5
23:22:00.76 +50:11:27.6
23:25:07.58 +54:12:38.1
23:39:19.81 +56:14:20.3
23:18:40.79 +52:55:57.3
23:30:55.38 +51:58:02.6
23:24:22.90 +50:20:34.9
23:25:33.09 +56:08:21.5
23:41:42.44 +54:39:45.5
23:53:53.39 +55:17:53.2
23:48:02.65 +56:26:08.5
23:31:05.16 +55:00:38.8
23:36:47.01 +55:28:07.8
23:47:25.88 +57:23:38.1
00:01:50.67 +55:27:32.4
00:16:51.06 +57:09:34.2
23:41:24.78 +55:36:49.5
23:48:28.52 +56:23:56.5
23:47:04.41 +51:55:58.8
23:55:29.15 +54:30:22.2
###################################################################################
23:46:50.97 +51:56:32.5 -- not an asteroid (will add it to exclusion list)
00:13:43.99 +54:31:40.9 -- not an asteroid (will add it to exclusion list)
23:56:31.16 +56:29:02.3 -- not an asteroid (will add it to exclusion list)
00:05:12.25 +51:03:42.6 -- not an asteroid (will add it to exclusion list)
23:43:27.49 +50:48:57.4 -- not an asteroid (will add it to exclusion list)
23:25:06.28 +54:08:56.6 -- not an asteroid (will add it to exclusion list)
23:31:29.79 +51:07:11.3 -- not an asteroid (will add it to exclusion list)
23:44:15.73 +54:03:03.6 -- not an asteroid (will add it to exclusion list)
23:36:02.75 +51:05:47.2 -- not an asteroid (will add it to exclusion list)
00:09:51.69 +55:21:40.4 -- not an asteroid (will add it to exclusion list)
23:44:35.93 +58:00:16.5 -- not an asteroid (will add it to exclusion list)
23:23:05.57 +54:06:19.4 -- not an asteroid (will add it to exclusion list)
23:19:48.01 +49:13:46.3 -- not an asteroid (will add it to exclusion list)
23:37:19.82 +57:11:47.8 -- not an asteroid (will add it to exclusion list)
23:33:42.96 +53:40:49.7 -- not an asteroid (will add it to exclusion list)
23:21:44.29 +53:21:19.0 -- not an asteroid (will add it to exclusion list)
23:43:01.12 +51:44:15.3 -- not an asteroid (will add it to exclusion list)
23:30:19.86 +51:32:15.6 -- not an asteroid (will add it to exclusion list)
23:45:40.11 +49:42:46.8 -- not an asteroid (will add it to exclusion list)
23:26:34.69 +52:38:37.3 -- not an asteroid (will add it to exclusion list)
23:32:48.72 +55:10:10.9 -- not an asteroid (will add it to exclusion list)
23:18:56.86 +52:58:26.6 -- not an asteroid (will add it to exclusion list)
00:04:18.17 +51:52:27.3 -- not an asteroid (will add it to exclusion list)
23:41:04.22 +54:08:50.8 -- not an asteroid (will add it to exclusion list)
23:14:21.20 +52:49:14.4 -- not an asteroid (will add it to exclusion list)
23:49:10.71 +51:58:44.7 -- not an asteroid (will add it to exclusion list)
23:43:00.68 +55:31:09.9 -- not an asteroid (will add it to exclusion list)
23:43:58.95 +55:38:50.8 -- not an asteroid (will add it to exclusion list)
00:26:38.45 +56:47:19.5 -- not an asteroid (will add it to exclusion list)
23:23:49.35 +54:57:28.0 -- not an asteroid (will add it to exclusion list)
23:34:26.31 +55:43:52.0 -- not an asteroid (will add it to exclusion list)
00:10:25.94 +58:05:06.9 -- not an asteroid (will add it to exclusion list)
23:14:57.96 +55:18:41.3 -- not an asteroid (will add it to exclusion list)
23:20:01.49 +56:18:40.6 -- not an asteroid (will add it to exclusion list)
23:40:38.95 +54:06:04.1 -- not an asteroid (will add it to exclusion list)
23:42:32.90 +58:08:11.3 -- not an asteroid (will add it to exclusion list)
23:27:20.61 +49:42:14.3 -- not an asteroid (will add it to exclusion list)
23:36:53.88 +55:39:27.7 -- not an asteroid (will add it to exclusion list)
23:44:34.08 +53:02:55.9 -- not an asteroid (will add it to exclusion list)
23:30:56.68 +51:10:37.0 -- not an asteroid (will add it to exclusion list)
23:33:59.07 +52:15:29.4 -- not an asteroid (will add it to exclusion list)
00:16:04.69 +54:40:19.5 -- not an asteroid (will add it to exclusion list)
23:46:23.31 +57:38:21.1 -- not an asteroid (will add it to exclusion list)
23:08:56.46 +57:15:29.7 -- not an asteroid (will add it to exclusion list)
23:15:24.67 +54:15:49.6 -- not an asteroid (will add it to exclusion list)
23:14:20.68 +56:26:27.3 -- not an asteroid (will add it to exclusion list)
00:00:15.41 +57:43:09.0 -- not an asteroid (will add it to exclusion list)
23:26:03.13 +52:03:35.9 -- not an asteroid (will add it to exclusion list)
23:45:47.83 +57:16:15.9 -- not an asteroid (will add it to exclusion list)
23:31:09.82 +52:06:27.4 -- not an asteroid (will add it to exclusion list)
23:16:41.18 +54:20:20.5 -- not an asteroid (will add it to exclusion list)
23:36:46.48 +53:03:10.3 -- not an asteroid (will add it to exclusion list)
23:51:14.19 +53:29:30.8 -- not an asteroid (will add it to exclusion list)
23:24:22.77 +57:21:09.2 -- not an asteroid (will add it to exclusion list)
23:10:31.41 +57:14:50.0 -- not an asteroid (will add it to exclusion list)
23:48:45.32 +54:05:07.7 -- not an asteroid (will add it to exclusion list)
23:16:25.73 +52:40:53.5 -- not an asteroid (will add it to exclusion list)
23:19:42.05 +51:36:25.9 -- not an asteroid (will add it to exclusion list)
00:32:19.53 +57:14:54.2 -- not an asteroid (will add it to exclusion list)
23:32:25.57 +51:54:36.9 -- not an asteroid (will add it to exclusion list)
23:16:35.53 +55:47:09.3 -- not an asteroid (will add it to exclusion list)
23:12:31.74 +56:42:50.5 -- not an asteroid (will add it to exclusion list)
23:45:04.37 +55:00:31.4 -- not an asteroid (will add it to exclusion list)
23:27:29.39 +55:44:25.2 -- not an asteroid (will add it to exclusion list)
00:11:49.65 +56:14:26.5 -- not an asteroid (will add it to exclusion list)
23:49:44.61 +55:38:29.7 -- not an asteroid (will add it to exclusion list)
23:41:51.68 +54:39:58.9 -- not an asteroid (will add it to exclusion list)
23:35:14.12 +56:30:57.6 -- not an asteroid (will add it to exclusion list)
23:25:47.99 +52:39:36.7 -- not an asteroid (will add it to exclusion list)
23:22:39.83 +57:01:55.9 -- not an asteroid (will add it to exclusion list)
23:46:34.36 +57:42:58.1 -- not an asteroid (will add it to exclusion list)
23:15:55.87 +53:32:18.6 -- not an asteroid (will add it to exclusion list)
00:18:51.07 +50:04:25.7 -- not an asteroid (will add it to exclusion list)
23:17:56.22 +50:57:32.0 -- not an asteroid (will add it to exclusion list)
23:22:04.88 +53:49:28.0 -- not an asteroid (will add it to exclusion list)
23:25:02.89 +56:51:11.0 -- not an asteroid (will add it to exclusion list)
23:12:15.38 +56:31:13.1 -- not an asteroid (will add it to exclusion list)
23:22:30.80 +52:04:54.8 -- not an asteroid (will add it to exclusion list)
23:30:34.79 +51:52:37.3 -- not an asteroid (will add it to exclusion list)
23:27:54.70 +55:41:49.2 -- not an asteroid (will add it to exclusion list)
23:19:17.20 +52:37:40.5 -- not an asteroid (will add it to exclusion list)
23:19:35.45 +54:16:30.4 -- not an asteroid (will add it to exclusion list)
23:40:37.12 +56:24:23.9 -- not an asteroid (will add it to exclusion list)
23:17:17.48 +55:08:01.9 -- not an asteroid (will add it to exclusion list)
23:37:42.13 +52:46:09.3 -- not an asteroid (will add it to exclusion list)
23:23:04.22 +52:29:55.9 -- not an asteroid (will add it to exclusion list)
23:13:33.87 +53:34:52.7 -- not an asteroid (will add it to exclusion list)
23:16:55.84 +55:40:34.4 -- not an asteroid (will add it to exclusion list)
23:39:41.70 +57:16:05.3 -- not an asteroid (will add it to exclusion list)
23:29:51.32 +56:20:02.2 -- not an asteroid (will add it to exclusion list)
23:18:41.24 +54:16:19.5 -- not an asteroid (will add it to exclusion list)
23:46:43.16 +50:45:04.7 -- not an asteroid (will add it to exclusion list)
23:28:05.73 +55:31:17.7 -- not an asteroid (will add it to exclusion list)
23:20:50.24 +57:13:06.3 -- not an asteroid (will add it to exclusion list)
23:12:44.76 +54:33:22.2 -- not an asteroid (will add it to exclusion list)
23:17:35.31 +54:08:15.4 -- not an asteroid (will add it to exclusion list)
23:56:33.04 +56:44:30.9 -- not an asteroid (will add it to exclusion list)
23:12:41.15 +54:49:13.2 -- not an asteroid (will add it to exclusion list)
23:18:56.50 +53:20:37.9 -- not an asteroid (will add it to exclusion list)
23:37:54.62 +52:32:03.2 -- not an asteroid (will add it to exclusion list)
23:21:14.39 +55:23:14.2 -- not an asteroid (will add it to exclusion list)
23:11:10.96 +55:59:33.2 -- not an asteroid (will add it to exclusion list)
23:38:08.00 +53:36:18.4 -- not an asteroid (will add it to exclusion list)
23:19:15.91 +51:56:02.6 -- not an asteroid (will add it to exclusion list)
23:50:25.76 +49:51:14.2 -- not an asteroid (will add it to exclusion list)
23:31:12.57 +53:30:57.7 -- not an asteroid (will add it to exclusion list)
23:31:08.95 +54:16:09.2 -- not an asteroid (will add it to exclusion list)
23:36:32.69 +50:40:34.5 -- not an asteroid (will add it to exclusion list)
23:23:09.38 +56:38:52.8 -- not an asteroid (will add it to exclusion list)
23:15:52.45 +52:57:57.3 -- not an asteroid (will add it to exclusion list)
23:21:37.62 +55:42:58.8 -- not an asteroid (will add it to exclusion list)
23:26:05.79 +53:11:06.1 -- not an asteroid (will add it to exclusion list)
23:27:06.61 +56:40:02.3 -- not an asteroid (will add it to exclusion list)
23:26:19.35 +51:13:14.5 -- not an asteroid (will add it to exclusion list)
23:19:40.15 +50:08:15.6 -- not an asteroid (will add it to exclusion list)
23:22:36.51 +57:23:01.3 -- not an asteroid (will add it to exclusion list)
23:25:41.45 +55:09:05.3 -- not an asteroid (will add it to exclusion list)
23:13:38.70 +53:34:21.6 -- not an asteroid (will add it to exclusion list)
23:29:11.90 +53:11:19.2 -- not an asteroid (will add it to exclusion list)
23:28:27.08 +51:42:39.1 -- not an asteroid (will add it to exclusion list)
23:58:05.32 +56:28:01.7 -- not an asteroid (will add it to exclusion list)
23:16:50.72 +52:05:37.3 -- not an asteroid (will add it to exclusion list)
23:34:22.93 +53:50:20.2 -- not an asteroid (will add it to exclusion list)
23:23:47.56 +54:34:21.7 -- not an asteroid (will add it to exclusion list)
23:31:35.90 +53:08:29.6 -- not an asteroid (will add it to exclusion list)
23:25:28.04 +49:20:13.5 -- not an asteroid (will add it to exclusion list)
23:43:15.02 +51:40:39.5 -- not an asteroid (will add it to exclusion list)
23:16:38.05 +55:10:33.8 -- not an asteroid (will add it to exclusion list)
23:30:32.18 +49:52:18.7 -- not an asteroid (will add it to exclusion list)
23:50:05.36 +50:49:19.3 -- not an asteroid (will add it to exclusion list)
23:26:00.27 +52:50:48.1 -- not an asteroid (will add it to exclusion list)
23:29:24.24 +51:40:00.7 -- not an asteroid (will add it to exclusion list)
23:34:39.79 +51:08:28.0 -- not an asteroid (will add it to exclusion list)
23:33:10.17 +56:17:31.8 -- not an asteroid (will add it to exclusion list)
23:11:51.57 +55:18:28.9 -- not an asteroid (will add it to exclusion list)
23:24:46.31 +54:53:45.7 -- not an asteroid (will add it to exclusion list)
23:17:29.43 +52:31:58.8 -- not an asteroid (will add it to exclusion list)
23:16:56.04 +51:46:16.2 -- not an asteroid (will add it to exclusion list)
23:36:48.14 +54:33:55.2 -- not an asteroid (will add it to exclusion list)
23:21:05.72 +55:55:41.1 -- not an asteroid (will add it to exclusion list)
23:12:51.33 +55:43:33.6 -- not an asteroid (will add it to exclusion list)
00:11:12.84 +57:36:28.0 -- not an asteroid (will add it to exclusion list)
23:35:48.19 +51:17:28.6 -- not an asteroid (will add it to exclusion list)
23:32:21.36 +53:10:40.3 -- not an asteroid (will add it to exclusion list)
23:29:15.19 +51:14:31.0 -- not an asteroid (will add it to exclusion list)
23:35:55.35 +53:26:18.6 -- not an asteroid (will add it to exclusion list)
23:22:52.50 +51:52:56.4 -- not an asteroid (will add it to exclusion list)
23:10:01.96 +57:27:59.1 -- not an asteroid (will add it to exclusion list)
23:27:13.52 +56:44:18.1 -- not an asteroid (will add it to exclusion list)
23:21:16.89 +53:23:06.9 -- not an asteroid (will add it to exclusion list)
23:28:33.41 +49:24:17.0 -- not an asteroid (will add it to exclusion list)
23:20:51.80 +51:28:43.2 -- not an asteroid (will add it to exclusion list)
00:07:17.65 +58:04:11.7 -- not an asteroid (will add it to exclusion list)
23:55:11.77 +54:35:56.4 -- not an asteroid (will add it to exclusion list)
23:42:05.76 +53:06:25.4 -- not an asteroid (will add it to exclusion list)
23:14:39.05 +57:15:47.4 -- not an asteroid (will add it to exclusion list)
00:10:04.69 +50:47:24.4 -- not an asteroid (will add it to exclusion list)
23:53:22.56 +56:58:21.9 -- not an asteroid (will add it to exclusion list)
23:15:47.66 +56:18:48.4 -- not an asteroid (will add it to exclusion list)
23:38:53.35 +51:52:36.4 -- not an asteroid (will add it to exclusion list)
23:26:58.61 +55:51:30.2 -- not an asteroid (will add it to exclusion list)
23:12:55.29 +55:44:24.2 -- not an asteroid (will add it to exclusion list)
23:44:00.08 +53:01:56.6 -- not an asteroid (will add it to exclusion list)
23:24:41.12 +50:44:55.6 -- not an asteroid (will add it to exclusion list)
23:23:53.43 +49:30:41.6 -- not an asteroid (will add it to exclusion list)
23:28:42.69 +54:24:51.9 -- not an asteroid (will add it to exclusion list)
23:15:33.52 +52:26:46.1 -- not an asteroid (will add it to exclusion list)
23:21:40.71 +53:15:15.5 -- not an asteroid (will add it to exclusion list)
23:42:00.42 +54:28:43.7 -- not an asteroid (will add it to exclusion list)
23:53:41.06 +51:21:14.9 -- not an asteroid (will add it to exclusion list)
23:51:17.09 +57:27:59.2 -- not an asteroid (will add it to exclusion list)
23:17:09.56 +56:05:57.0 -- not an asteroid (will add it to exclusion list)
23:24:47.36 +51:03:21.4 -- not an asteroid (will add it to exclusion list)
23:10:21.25 +56:59:48.6 -- not an asteroid (will add it to exclusion list)
23:24:46.68 +52:18:02.5 -- not an asteroid (will add it to exclusion list)
23:21:20.30 +49:31:45.4 -- not an asteroid (will add it to exclusion list)
23:30:41.74 +57:06:29.4 -- not an asteroid (will add it to exclusion list)
23:22:49.28 +56:16:31.4 -- not an asteroid (will add it to exclusion list)
23:27:30.19 +54:55:09.7 -- not an asteroid (will add it to exclusion list)
23:19:00.00 +52:31:08.7 -- not an asteroid (will add it to exclusion list)
23:24:44.80 +53:30:14.1 -- not an asteroid (will add it to exclusion list)
23:11:37.88 +55:12:40.4 -- not an asteroid (will add it to exclusion list)
23:49:31.85 +52:38:02.7 -- not an asteroid (will add it to exclusion list)
23:26:36.90 +50:52:54.8 -- not an asteroid (will add it to exclusion list)
23:34:40.85 +54:45:09.4 -- not an asteroid (will add it to exclusion list)
23:23:15.10 +53:50:12.7 -- not an asteroid (will add it to exclusion list)
23:18:37.91 +55:18:04.0 -- not an asteroid (will add it to exclusion list)
23:33:53.96 +51:29:45.2 -- not an asteroid (will add it to exclusion list)
23:47:50.81 +51:54:48.6 -- not an asteroid (will add it to exclusion list)
23:27:46.31 +56:30:45.6 -- not an asteroid (will add it to exclusion list)
00:03:20.01 +57:13:23.6 -- not an asteroid (will add it to exclusion list)
23:30:12.31 +55:03:27.7 -- not an asteroid (will add it to exclusion list)
23:19:35.87 +56:55:08.6 -- not an asteroid (will add it to exclusion list)
23:30:08.69 +52:34:41.0 -- not an asteroid (will add it to exclusion list)
23:33:32.25 +55:22:41.6 -- not an asteroid (will add it to exclusion list)
23:19:08.81 +57:15:13.4 -- not an asteroid (will add it to exclusion list)
23:47:13.67 +57:22:32.7 -- not an asteroid (will add it to exclusion list)
23:46:36.09 +57:25:52.7 -- not an asteroid (will add it to exclusion list)
23:14:14.72 +52:54:28.7 -- not an asteroid (will add it to exclusion list)
23:33:16.07 +53:01:37.5 -- not an asteroid (will add it to exclusion list)
23:22:00.76 +50:11:27.6 -- not an asteroid (will add it to exclusion list)
23:25:07.58 +54:12:38.1 -- not an asteroid (will add it to exclusion list)
23:39:19.81 +56:14:20.3 -- not an asteroid (will add it to exclusion list)
23:18:40.79 +52:55:57.3 -- not an asteroid (will add it to exclusion list)
23:30:55.38 +51:58:02.6 -- not an asteroid (will add it to exclusion list)
23:24:22.90 +50:20:34.9 -- not an asteroid (will add it to exclusion list)
23:25:33.09 +56:08:21.5 -- not an asteroid (will add it to exclusion list)
23:41:42.44 +54:39:45.5 -- not an asteroid (will add it to exclusion list)
23:53:53.39 +55:17:53.2 -- not an asteroid (will add it to exclusion list)
23:48:02.65 +56:26:08.5 -- not an asteroid (will add it to exclusion list)
23:31:05.16 +55:00:38.8 -- not an asteroid (will add it to exclusion list)
23:36:47.01 +55:28:07.8 -- not an asteroid (will add it to exclusion list)
23:47:25.88 +57:23:38.1 -- not an asteroid (will add it to exclusion list)
00:01:50.67 +55:27:32.4 -- not an asteroid (will add it to exclusion list)
00:16:51.06 +57:09:34.2 -- not an asteroid (will add it to exclusion list)
23:41:24.78 +55:36:49.5 -- not an asteroid (will add it to exclusion list)
23:48:28.52 +56:23:56.5 -- not an asteroid (will add it to exclusion list)
23:47:04.41 +51:55:58.8 -- not an asteroid (will add it to exclusion list)
23:55:29.15 +54:30:22.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:15.41 +57:43:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:50.67 +55:27:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:20.01 +57:13:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:18.17 +51:52:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:12.25 +51:03:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:17.65 +58:04:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:51.69 +55:21:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:04.69 +50:47:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:25.94 +58:05:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:12.84 +57:36:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:49.65 +56:14:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:43.99 +54:31:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:04.69 +54:40:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:51.06 +57:09:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:51.07 +50:04:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:38.45 +56:47:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:19.53 +57:14:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:56.46 +57:15:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:01.96 +57:27:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:21.25 +56:59:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:31.41 +57:14:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:10.96 +55:59:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:37.88 +55:12:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:51.57 +55:18:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:15.38 +56:31:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:31.74 +56:42:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:41.15 +54:49:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:44.76 +54:33:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:51.33 +55:43:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:55.29 +55:44:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:33.87 +53:34:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:38.70 +53:34:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:14.72 +52:54:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:20.68 +56:26:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:21.20 +52:49:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:39.05 +57:15:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:57.96 +55:18:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:24.67 +54:15:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:33.52 +52:26:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:47.66 +56:18:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:52.45 +52:57:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:55.87 +53:32:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:25.73 +52:40:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:35.53 +55:47:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:38.05 +55:10:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:41.18 +54:20:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:50.72 +52:05:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:55.84 +55:40:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:56.04 +51:46:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:09.56 +56:05:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:17.48 +55:08:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:29.43 +52:31:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:35.31 +54:08:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:56.22 +50:57:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:37.91 +55:18:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:40.79 +52:55:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:41.24 +54:16:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.50 +53:20:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.86 +52:58:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:00.00 +52:31:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:08.81 +57:15:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:15.91 +51:56:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:17.20 +52:37:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:35.45 +54:16:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:35.87 +56:55:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:40.15 +50:08:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:42.05 +51:36:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:48.01 +49:13:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:01.49 +56:18:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:50.24 +57:13:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:51.80 +51:28:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:05.72 +55:55:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:14.39 +55:23:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:16.89 +53:23:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:20.30 +49:31:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:37.62 +55:42:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:40.71 +53:15:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:44.29 +53:21:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:00.76 +50:11:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:04.88 +53:49:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:30.80 +52:04:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:36.51 +57:23:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:39.83 +57:01:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:49.28 +56:16:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:52.50 +51:52:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:04.22 +52:29:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:05.57 +54:06:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:09.38 +56:38:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:15.10 +53:50:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:47.56 +54:34:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:49.35 +54:57:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:53.43 +49:30:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:22.77 +57:21:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:22.90 +50:20:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:41.12 +50:44:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:44.80 +53:30:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:46.31 +54:53:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:46.68 +52:18:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:47.36 +51:03:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:02.89 +56:51:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:06.28 +54:08:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:07.58 +54:12:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:28.04 +49:20:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:33.09 +56:08:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:41.45 +55:09:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:47.99 +52:39:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:00.27 +52:50:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:03.13 +52:03:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:05.79 +53:11:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:19.35 +51:13:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:34.69 +52:38:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:36.90 +50:52:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:58.61 +55:51:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:06.61 +56:40:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:13.52 +56:44:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:20.61 +49:42:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:29.39 +55:44:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:30.19 +54:55:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:46.31 +56:30:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:54.70 +55:41:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:05.73 +55:31:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:27.08 +51:42:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:33.41 +49:24:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:42.69 +54:24:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:11.90 +53:11:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:15.19 +51:14:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:24.24 +51:40:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:51.32 +56:20:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:08.69 +52:34:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:12.31 +55:03:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:19.86 +51:32:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:32.18 +49:52:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:34.79 +51:52:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:41.74 +57:06:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:55.38 +51:58:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:56.68 +51:10:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:05.16 +55:00:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:08.95 +54:16:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:09.82 +52:06:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:12.57 +53:30:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:29.79 +51:07:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:35.90 +53:08:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:21.36 +53:10:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:25.57 +51:54:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:48.72 +55:10:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:10.17 +56:17:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:16.07 +53:01:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:32.25 +55:22:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:42.96 +53:40:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:53.96 +51:29:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:59.07 +52:15:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:22.93 +53:50:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:26.31 +55:43:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:39.79 +51:08:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:40.85 +54:45:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:14.12 +56:30:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:48.19 +51:17:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:55.35 +53:26:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:02.75 +51:05:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:32.69 +50:40:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:46.48 +53:03:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:47.01 +55:28:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:48.14 +54:33:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:53.88 +55:39:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:19.82 +57:11:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:42.13 +52:46:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:54.62 +52:32:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:08.00 +53:36:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:53.35 +51:52:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:19.81 +56:14:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:41.70 +57:16:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:37.12 +56:24:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:38.95 +54:06:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:04.22 +54:08:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:24.78 +55:36:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:42.44 +54:39:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:51.68 +54:39:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:00.42 +54:28:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:05.76 +53:06:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:32.90 +58:08:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:00.68 +55:31:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:01.12 +51:44:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:15.02 +51:40:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:27.49 +50:48:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:58.95 +55:38:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:00.08 +53:01:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:15.73 +54:03:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:34.08 +53:02:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:35.93 +58:00:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:04.37 +55:00:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:40.11 +49:42:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:47.83 +57:16:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:23.31 +57:38:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:34.36 +57:42:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:36.09 +57:25:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:43.16 +50:45:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:50.97 +51:56:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:04.41 +51:55:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:13.67 +57:22:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:25.88 +57:23:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:50.81 +51:54:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:02.65 +56:26:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:28.52 +56:23:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:45.32 +54:05:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:10.71 +51:58:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:31.85 +52:38:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:44.61 +55:38:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:05.36 +50:49:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:25.76 +49:51:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:14.19 +53:29:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:17.09 +57:27:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:22.56 +56:58:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:41.06 +51:21:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:53.39 +55:17:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:11.77 +54:35:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:29.15 +54:30:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:31.16 +56:29:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:33.04 +56:44:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:05.32 +56:28:01.7 -- 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)
00:00:15.41 +57:43:09.0 -- not a known variable star
00:01:50.67 +55:27:32.4 -- not a known variable star
00:03:20.01 +57:13:23.6 -- a known variable star
00:04:18.17 +51:52:27.3 -- not a known variable star
00:05:12.25 +51:03:42.6 -- not a known variable star
00:07:17.65 +58:04:11.7 -- not a known variable star
00:09:51.69 +55:21:40.4 -- a known variable star
00:10:04.69 +50:47:24.4 -- not a known variable star
00:10:25.94 +58:05:06.9 -- not a known variable star
00:11:12.84 +57:36:28.0 -- not a known variable star
00:11:49.65 +56:14:26.5 -- not a known variable star
00:13:43.99 +54:31:40.9 -- not a known variable star
00:16:04.69 +54:40:19.5 -- a known variable star
00:16:51.06 +57:09:34.2 -- not a known variable star
00:18:51.07 +50:04:25.7 -- a known variable star
00:26:38.45 +56:47:19.5 -- not a known variable star
00:32:19.53 +57:14:54.2 -- not a known variable star
23:08:56.46 +57:15:29.7 -- not a known variable star
23:10:01.96 +57:27:59.1 -- not a known variable star
23:10:21.25 +56:59:48.6 -- not a known variable star
23:10:31.41 +57:14:50.0 -- not a known variable star
23:11:10.96 +55:59:33.2 -- a known variable star
23:11:37.88 +55:12:40.4 -- not a known variable star
23:11:51.57 +55:18:28.9 -- a known variable star
23:12:15.38 +56:31:13.1 -- not a known variable star
23:12:31.74 +56:42:50.5 -- not a known variable star
23:12:41.15 +54:49:13.2 -- not a known variable star
23:12:44.76 +54:33:22.2 -- not a known variable star
23:12:51.33 +55:43:33.6 -- a known variable star
23:12:55.29 +55:44:24.2 -- not a known variable star
23:13:33.87 +53:34:52.7 -- not a known variable star
23:13:38.70 +53:34:21.6 -- not a known variable star
23:14:14.72 +52:54:28.7 -- not a known variable star
23:14:20.68 +56:26:27.3 -- not a known variable star
23:14:21.20 +52:49:14.4 -- not a known variable star
23:14:39.05 +57:15:47.4 -- not a known variable star
23:14:57.96 +55:18:41.3 -- a known variable star
23:15:24.67 +54:15:49.6 -- a known variable star
23:15:33.52 +52:26:46.1 -- not a known variable star
23:15:47.66 +56:18:48.4 -- not a known variable star
23:15:52.45 +52:57:57.3 -- not a known variable star
23:15:55.87 +53:32:18.6 -- not a known variable star
23:16:25.73 +52:40:53.5 -- not a known variable star
23:16:35.53 +55:47:09.3 -- a known variable star
23:16:38.05 +55:10:33.8 -- not a known variable star
23:16:41.18 +54:20:20.5 -- not a known variable star
23:16:50.72 +52:05:37.3 -- not a known variable star
23:16:55.84 +55:40:34.4 -- not a known variable star
23:16:56.04 +51:46:16.2 -- a known variable star
23:17:09.56 +56:05:57.0 -- not a known variable star
23:17:17.48 +55:08:01.9 -- not a known variable star
23:17:29.43 +52:31:58.8 -- not a known variable star
23:17:35.31 +54:08:15.4 -- not a known variable star
23:17:56.22 +50:57:32.0 -- not a known variable star
23:18:37.91 +55:18:04.0 -- not a known variable star
23:18:40.79 +52:55:57.3 -- not a known variable star
23:18:41.24 +54:16:19.5 -- not a known variable star
23:18:56.50 +53:20:37.9 -- a known variable star
23:18:56.86 +52:58:26.6 -- not a known variable star
23:19:00.00 +52:31:08.7 -- not a known variable star
23:19:08.81 +57:15:13.4 -- not a known variable star
23:19:15.91 +51:56:02.6 -- a known variable star
23:19:17.20 +52:37:40.5 -- a known variable star
23:19:35.45 +54:16:30.4 -- not a known variable star
23:19:35.87 +56:55:08.6 -- not a known variable star
23:19:40.15 +50:08:15.6 -- not a known variable star
23:19:42.05 +51:36:25.9 -- a known variable star
23:19:48.01 +49:13:46.3 -- not a known variable star
23:20:01.49 +56:18:40.6 -- a known variable star
23:20:50.24 +57:13:06.3 -- not a known variable star
23:20:51.80 +51:28:43.2 -- not a known variable star
23:21:05.72 +55:55:41.1 -- not a known variable star
23:21:14.39 +55:23:14.2 -- not a known variable star
23:21:16.89 +53:23:06.9 -- not a known variable star
23:21:20.30 +49:31:45.4 -- not a known variable star
23:21:37.62 +55:42:58.8 -- not a known variable star
23:21:40.71 +53:15:15.5 -- not a known variable star
23:21:44.29 +53:21:19.0 -- not a known variable star
23:22:00.76 +50:11:27.6 -- not a known variable star
23:22:04.88 +53:49:28.0 -- not a known variable star
23:22:30.80 +52:04:54.8 -- not a known variable star
23:22:36.51 +57:23:01.3 -- not a known variable star
23:22:39.83 +57:01:55.9 -- not a known variable star
23:22:49.28 +56:16:31.4 -- a known variable star
23:22:52.50 +51:52:56.4 -- not a known variable star
23:23:04.22 +52:29:55.9 -- not a known variable star
23:23:05.57 +54:06:19.4 -- not a known variable star
23:23:09.38 +56:38:52.8 -- not a known variable star
23:23:15.10 +53:50:12.7 -- not a known variable star
23:23:47.56 +54:34:21.7 -- a known variable star
23:23:49.35 +54:57:28.0 -- not a known variable star
23:23:53.43 +49:30:41.6 -- not a known variable star
23:24:22.77 +57:21:09.2 -- a known variable star
23:24:22.90 +50:20:34.9 -- not a known variable star
23:24:41.12 +50:44:55.6 -- a known variable star
23:24:44.80 +53:30:14.1 -- not a known variable star
23:24:46.31 +54:53:45.7 -- not a known variable star
23:24:46.68 +52:18:02.5 -- not a known variable star
23:24:47.36 +51:03:21.4 -- not a known variable star
23:25:02.89 +56:51:11.0 -- not a known variable star
23:25:06.28 +54:08:56.6 -- not a known variable star
23:25:07.58 +54:12:38.1 -- not a known variable star
23:25:28.04 +49:20:13.5 -- not a known variable star
23:25:33.09 +56:08:21.5 -- not a known variable star
23:25:41.45 +55:09:05.3 -- not a known variable star
23:25:47.99 +52:39:36.7 -- not a known variable star
23:26:00.27 +52:50:48.1 -- not a known variable star
23:26:03.13 +52:03:35.9 -- not a known variable star
23:26:05.79 +53:11:06.1 -- not a known variable star
23:26:19.35 +51:13:14.5 -- not a known variable star
23:26:34.69 +52:38:37.3 -- not a known variable star
23:26:36.90 +50:52:54.8 -- a known variable star
23:26:58.61 +55:51:30.2 -- not a known variable star
23:27:06.61 +56:40:02.3 -- a known variable star
23:27:13.52 +56:44:18.1 -- not a known variable star
23:27:20.61 +49:42:14.3 -- not a known variable star
23:27:29.39 +55:44:25.2 -- not a known variable star
23:27:30.19 +54:55:09.7 -- not a known variable star
23:27:46.31 +56:30:45.6 -- a known variable star
23:27:54.70 +55:41:49.2 -- not a known variable star
23:28:05.73 +55:31:17.7 -- not a known variable star
23:28:27.08 +51:42:39.1 -- not a known variable star
23:28:33.41 +49:24:17.0 -- not a known variable star
23:28:42.69 +54:24:51.9 -- not a known variable star
23:29:11.90 +53:11:19.2 -- not a known variable star
23:29:15.19 +51:14:31.0 -- not a known variable star
23:29:24.24 +51:40:00.7 -- not a known variable star
23:29:51.32 +56:20:02.2 -- not a known variable star
23:30:08.69 +52:34:41.0 -- not a known variable star
23:30:12.31 +55:03:27.7 -- not a known variable star
23:30:19.86 +51:32:15.6 -- a known variable star
23:30:32.18 +49:52:18.7 -- not a known variable star
23:30:34.79 +51:52:37.3 -- not a known variable star
23:30:41.74 +57:06:29.4 -- not a known variable star
23:30:55.38 +51:58:02.6 -- not a known variable star
23:30:56.68 +51:10:37.0 -- not a known variable star
23:31:05.16 +55:00:38.8 -- not a known variable star
23:31:08.95 +54:16:09.2 -- not a known variable star
23:31:09.82 +52:06:27.4 -- not a known variable star
23:31:12.57 +53:30:57.7 -- not a known variable star
23:31:29.79 +51:07:11.3 -- a known variable star
23:31:35.90 +53:08:29.6 -- not a known variable star
23:32:21.36 +53:10:40.3 -- not a known variable star
23:32:25.57 +51:54:36.9 -- a known variable star
23:32:48.72 +55:10:10.9 -- not a known variable star
23:33:10.17 +56:17:31.8 -- a known variable star
23:33:16.07 +53:01:37.5 -- a known variable star
23:33:32.25 +55:22:41.6 -- not a known variable star
23:33:42.96 +53:40:49.7 -- not a known variable star
23:33:53.96 +51:29:45.2 -- not a known variable star
23:33:59.07 +52:15:29.4 -- not a known variable star
23:34:22.93 +53:50:20.2 -- not a known variable star
23:34:26.31 +55:43:52.0 -- a known variable star
23:34:39.79 +51:08:28.0 -- not a known variable star
23:34:40.85 +54:45:09.4 -- not a known variable star
23:35:14.12 +56:30:57.6 -- not a known variable star
23:35:48.19 +51:17:28.6 -- not a known variable star
23:35:55.35 +53:26:18.6 -- not a known variable star
23:36:02.75 +51:05:47.2 -- a known variable star
23:36:32.69 +50:40:34.5 -- not a known variable star
23:36:46.48 +53:03:10.3 -- not a known variable star
23:36:47.01 +55:28:07.8 -- not a known variable star
23:36:48.14 +54:33:55.2 -- not a known variable star
23:36:53.88 +55:39:27.7 -- not a known variable star
23:37:19.82 +57:11:47.8 -- not a known variable star
23:37:42.13 +52:46:09.3 -- a known variable star
23:37:54.62 +52:32:03.2 -- not a known variable star
23:38:08.00 +53:36:18.4 -- not a known variable star
23:38:53.35 +51:52:36.4 -- not a known variable star
23:39:19.81 +56:14:20.3 -- not a known variable star
23:39:41.70 +57:16:05.3 -- a known variable star
23:40:37.12 +56:24:23.9 -- a known variable star
23:40:38.95 +54:06:04.1 -- not a known variable star
23:41:04.22 +54:08:50.8 -- not a known variable star
23:41:24.78 +55:36:49.5 -- not a known variable star
23:41:42.44 +54:39:45.5 -- a known variable star
23:41:51.68 +54:39:58.9 -- not a known variable star
23:42:00.42 +54:28:43.7 -- not a known variable star
23:42:05.76 +53:06:25.4 -- not a known variable star
23:42:32.90 +58:08:11.3 -- not a known variable star
23:43:00.68 +55:31:09.9 -- not a known variable star
23:43:01.12 +51:44:15.3 -- a known variable star
23:43:15.02 +51:40:39.5 -- not a known variable star
23:43:27.49 +50:48:57.4 -- a known variable star
23:43:58.95 +55:38:50.8 -- not a known variable star
23:44:00.08 +53:01:56.6 -- not a known variable star
23:44:15.73 +54:03:03.6 -- not a known variable star
23:44:34.08 +53:02:55.9 -- not a known variable star
23:44:35.93 +58:00:16.5 -- not a known variable star
23:45:04.37 +55:00:31.4 -- not a known variable star
23:45:40.11 +49:42:46.8 -- a known variable star
23:45:47.83 +57:16:15.9 -- not a known variable star
23:46:23.31 +57:38:21.1 -- not a known variable star
23:46:34.36 +57:42:58.1 -- not a known variable star
23:46:36.09 +57:25:52.7 -- not a known variable star
23:46:43.16 +50:45:04.7 -- not a known variable star
23:46:50.97 +51:56:32.5 -- not a known variable star
23:47:04.41 +51:55:58.8 -- not a known variable star
23:47:13.67 +57:22:32.7 -- not a known variable star
23:47:25.88 +57:23:38.1 -- not a known variable star
23:47:50.81 +51:54:48.6 -- not a known variable star
23:48:02.65 +56:26:08.5 -- a known variable star
23:48:28.52 +56:23:56.5 -- a known variable star
23:48:45.32 +54:05:07.7 -- not a known variable star
23:49:10.71 +51:58:44.7 -- not a known variable star
23:49:31.85 +52:38:02.7 -- not a known variable star
23:49:44.61 +55:38:29.7 -- not a known variable star
23:50:05.36 +50:49:19.3 -- not a known variable star
23:50:25.76 +49:51:14.2 -- not a known variable star
23:51:14.19 +53:29:30.8 -- not a known variable star
23:51:17.09 +57:27:59.2 -- not a known variable star
23:53:22.56 +56:58:21.9 -- not a known variable star
23:53:41.06 +51:21:14.9 -- not a known variable star
23:53:53.39 +55:17:53.2 -- not a known variable star
23:55:11.77 +54:35:56.4 -- not a known variable star
23:55:29.15 +54:30:22.2 -- not a known variable star
23:56:31.16 +56:29:02.3 -- not a known variable star
23:56:33.04 +56:44:30.9 -- a known variable star
23:58:05.32 +56:28:01.7 -- a known variable star
Found 178 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
219 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 219 (excluding asteroids and hot pixels, 178 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)2461255.65741605 -observatory V36
07:30:12.43 +20:12:12.9 Mercury (0.1mag)
11:44:39.69 +01:25:57.1 Venus (-4.3mag)
05:34:29.18 +23:25:39.3 Mars (1.3mag)
08:38:21.84 +18:58:04.5 Jupiter (-1.8mag)
00:56:41.91 +03:18:36.9 Saturn (0.6mag)
04:11:06.53 +20:55:20.3 Uranus (5.8mag)
00:16:22.31 +00:15:09.6 Neptune (7.7mag)
20:28:37.77 -23:28:11.2 Pluto (14.4mag)
00:11:25.91 +03:35:36.8 Moon (-11.3mag)
-rw-r--r-- 1 apache apache 362 Aug 2 23:11 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461255.65741605:
08:38:19.64 +18:58:13.5 Io (6.0mag)
08:38:13.47 +18:58:40.7 Europa (6.3mag)
08:38:20.96 +18:58:05.7 Ganymede (5.6mag)
08:37:55.88 +18:59:52.7 Callisto (6.7mag)
08:36:01.69 +18:54:24.8 Himalia (15.7mag)
08:38:26.12 +18:57:47.0 Thebe (16.6mag)
08:35:30.30 +18:53:56.5 Elara (17.7mag)
08:42:25.75 +18:39:57.7 Pasiphae (17.9mag)
08:41:52.64 +19:07:16.5 Carme (19.0mag)
00:56:52.31 +03:18:41.9 Titan (8.4mag)
00:56:42.06 +03:18:19.6 Rhea (9.7mag)
00:56:36.71 +03:16:30.5 Iapetus (11.2mag)
00:56:40.23 +03:19:05.2 Hyperion (14.4mag)
00:56:10.95 +03:12:28.3 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 2 23:11 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461255.65741605:
18:44:42.49 -25:28:19.8 JWST
16:19:52.41 +50:04:56.7 Chandra
20:05:19.84 +23:57:59.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 2 23:11 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461255.65741605 -observatory V36
03:07:46.02 +16:56:09.3 17.7mag P/1996 R2 (Lagerkvist)
18:03:31.11 -34:39:01.5 13.9mag P/2010 H2 (Vales)
06:49:01.34 -68:43:19.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:08:25.77 +32:53:18.6 17.7mag C/2017 K2 (PANSTARRS)
03:28:04.52 +35:07:28.5 16.5mag P/2021 N1 (ZTF)
22:42:44.94 +31:43:29.4 17.3mag C/2022 E2 (ATLAS)
06:38:21.44 +26:37:33.0 16.8mag C/2022 N2 (PANSTARRS)
10:16:53.48 +28:41:55.4 16.9mag C/2022 QE78 (ATLAS)
09:25:27.72 +05:16:56.2 17.9mag C/2022 R6 (PANSTARRS)
15:11:44.91 -12:05:39.0 17.9mag P/2023 B1 (PANSTARRS)
21:17:34.93 +66:31:41.3 17.9mag C/2023 H5 (Lemmon)
15:53:19.95 -12:27:32.4 14.3mag C/2023 R1 (PANSTARRS)
08:02:18.75 +31:07:07.1 15.2mag C/2024 E1 (Wierzchos)
15:07:54.77 +15:37:12.6 17.7mag C/2024 G6 (ATLAS)
19:09:39.73 +42:44:02.2 13.7mag C/2024 J3 (ATLAS)
21:18:05.21 +48:50:51.1 17.6mag C/2024 R4 (PANSTARRS)
05:10:59.30 -13:02:33.9 15.5mag C/2024 T5 (ATLAS)
06:52:49.79 +25:02:29.7 17.9mag C/2025 J1 (Borisov)
07:28:31.51 -15:27:47.9 17.6mag C/2025 R3 (PANSTARRS)
10:25:57.01 +21:13:02.2 17.4mag C/2025 V2 (Rankin)
12:55:11.87 +02:40:39.6 17.0mag C/2025 Y1 (ATLAS)
16:05:32.77 +78:16:47.9 16.9mag C/2026 A2 (Bok)
03:05:17.73 +46:04:20.9 17.0mag C/2026 B2 (Sun-Gao)
11:42:40.69 +07:59:10.4 17.2mag A/2026 E1
21:52:31.12 -25:07:02.1 6.9mag 10P/Tempel
11:25:58.37 -03:05:39.0 16.2mag 29P/Schwassmann-Wachmann
04:32:51.42 +31:58:25.5 18.0mag 47P/Ashbrook-Jackson
10:57:20.19 +06:18:02.5 17.2mag 63P/Wild
00:54:15.87 -05:17:01.8 15.5mag 65P/Gunn
05:23:56.78 +20:45:20.0 13.7mag 78P/Gehrels
20:42:33.70 -22:55:37.6 17.9mag 84P/Giclas
02:55:24.15 +13:17:13.4 16.6mag 88P/Howell
07:42:44.00 +28:19:13.9 16.1mag 93P/Lovas
03:52:16.92 +14:54:51.8 17.7mag 112P/Urata-Niijima
05:39:40.67 +30:46:38.6 16.4mag 114P/Wiseman-Skiff
09:06:25.51 +27:29:03.7 15.0mag 123P/West-Hartley
11:33:40.43 -08:18:33.1 17.0mag 124P/Mrkos
05:28:59.67 +21:11:06.9 16.1mag 128P/Shoemaker-Holt
06:19:44.61 +19:07:47.5 17.9mag 131P/Mueller
00:04:01.13 +03:25:49.6 17.6mag 139P/Vaisala-Oterma
03:22:06.69 -19:52:21.4 14.2mag 161P/Hartley-IRAS
06:58:29.42 +37:28:13.8 15.7mag 162P/SidingSpring
16:37:12.56 +36:26:37.6 12.6mag 169P/NEAT
02:33:24.02 +09:23:15.3 17.6mag 220P/McNaught
16:39:14.00 -09:43:40.9 17.6mag 235P/LINEAR
20:25:58.98 -52:47:31.5 17.8mag 259P/Garradd
03:07:20.72 +22:59:25.9 15.4mag 260P/McNaught
06:50:00.67 +37:46:59.8 17.3mag 295P/LINEAR
15:09:00.12 +03:41:30.9 17.7mag 391P/Kowalski
08:56:15.35 +18:37:18.4 17.9mag 450P/LONEOS
08:28:12.33 +37:10:47.4 18.0mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
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
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 2 23:11 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:54:08.534 -07:13:49.93 AT 2026uqz 2026-07-10.09 21.3674
21:08:30.722 -24:28:14.91 AT 2026uqy 2026-07-10.34 22.6821
19:36:58.373 -21:42:17.03 AT 2026uqx 2026-07-09.23 23.159
20:44:07.484 -21:01:35.00 AT 2026uqw 2026-07-09.31 23.0996
19:38:33.301 -21:29:24.48 AT 2026uqv 2026-07-09.23 23.3974
19:53:21.622 -21:02:37.45 AT 2026uqu 2026-07-09.24 22.9664
19:51:47.480 -21:22:43.49 AT 2026uqt 2026-07-09.24 23.0505
19:48:33.045 -21:19:41.03 AT 2026uqs 2026-07-09.23 23.2639
21:38:33.144 -17:23:10.17 AT 2026uqr 2026-07-09.29 23.2028
19:30:17.464 -19:22:43.60 AT 2026uqq 2026-07-09.26 22.9316
03:49:20.579 -48:35:22.65 AT 2026uqp 2026-07-09.42 22.9951
21:29:22.607 -18:53:04.27 AT 2026uqo 2026-07-09.29 23.2945
00:36:53.932 -44:10:51.43 AT 2026uqn 2026-07-09.41 23.8057
19:59:10.521 -19:34:34.05 AT 2026uqm 2026-07-09.24 23.1419
20:00:57.808 -19:42:57.80 AT 2026uql 2026-07-09.24 22.6536
20:01:28.696 -18:37:38.63 AT 2026uqk 2026-07-09.24 23.3834
19:54:33.149 -19:25:04.99 AT 2026uqj 2026-07-09.24 22.0922
19:38:52.087 -21:51:55.98 AT 2026uqi 2026-07-09.23 22.4832
19:58:31.188 -18:21:40.63 AT 2026uqh 2026-07-09.24 23.1243
19:23:39.486 -23:20:09.61 AT 2026uqg 2026-07-09.33 22.6417
-rw-r--r-- 1 apache apache 88K Aug 2 23:11 tns_transients_list.txt
