This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV
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 05 26.2012 2461186.7012 11.16 19:13:51.54 +02:07:15.2
37.38453 -4.01367 galactic Aql Second-epoch detections are separated by 4.7" and 2.3 pix
The object was found in VSX 3" ASASSN-V J191351.67+020712.5
Type: SRS
# Max. Min./Amp. JD0 Period
13.260 V 13.430 V 2457449.13200 24.222000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:51.54 +02:07:15.2: 12.50 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:51.54 +02:07:15.2: 12.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191351.67+020712.5,2461186.7012,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191351.67+020712.5 20260526.2012 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 05 26.2012 2461186.7012 11.69 19:20:37.79 +04:38:35.2
40.41024 -4.34560 galactic Aql Second-epoch detections are separated by 2.8" and 2.1 pix
The object was found in VSX 5" ASASSN-V J192038.12+043834.0
Type: SRS
# Max. Min./Amp. JD0 Period
13.910 V 14.130 V 2457899.02500 24.643000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:20:37.79 +04:38:35.2: 12.87 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:20:37.79 +04:38:35.2: 12.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192038.12+043834.0,2461186.7012,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192038.12+043834.0 20260526.2012 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 05 26.2012 2461186.7012 11.61 19:16:08.18 +03:15:01.8
38.65222 -3.99773 galactic Aql Second-epoch detections are separated by 1.5" and 2.1 pix
The object was found in VSX 7" Gaia DR3 4292225461896275584
Type:
# Max. Min./Amp. JD0 Period
19.350 G 19.680 G 0.495047000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:08.18 +03:15:01.8: 12.63 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:08.18 +03:15:01.8: 12.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4292225461896275584,2461186.7012,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4292225461896275584 20260526.2012 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.40 19:10:18.03 +00:51:17.2
35.84791 -3.80471 galactic Aql Second-epoch detections are separated by 4.5" and 1.7 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 J287.5836+00.8487 | 19:10:17.96 +00:51:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.990+/-0.033 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:18.03 +00:51:17.2: 12.60 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:18.03 +00:51:17.2: 12.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.5836+00.8487,2461186.7012,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.5836+00.8487 20260526.2012 11.40CV 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 05 26.2012 2461186.7012 11.47 19:08:31.32 +00:59:05.4
35.75977 -3.34994 galactic Aql Second-epoch detections are separated by 2.7" and 2.0 pix
The object was found in VSX 6" Gaia DR3 4267376224255204224
Type:
# Max. Min./Amp. JD0 Period
18.210 G 18.700 G
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:31.32 +00:59:05.4: 12.62 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:31.32 +00:59:05.4: 12.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267376224255204224,2461186.7012,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267376224255204224 20260526.2012 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 05 26.2012 2461186.7012 10.82 19:16:36.52 +02:39:51.6
38.18542 -4.37291 galactic Aql Second-epoch detections are separated by 2.1" 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 J289.1410+02.6627 | 19:16:36.60 +02:39:49.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.118+/-0.040 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:36.52 +02:39:51.6: 11.74 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:36.52 +02:39:51.6: 11.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.1410+02.6627,2461186.7012,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.1410+02.6627 20260526.2012 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.74 18:39:14.92 +08:50:13.6
39.45191 6.70755 galactic Oph Second-epoch detections are separated by 2.8" and 1.9 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 J279.8125+08.8366 | 18:39:15.02 +08:50:11.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.182+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:39:14.92 +08:50:13.6: 12.71 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:39:14.92 +08:50:13.6: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J279.8125+08.8366,2461186.7012,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J279.8125+08.8366 20260526.2012 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.42 19:09:40.50 +01:11:06.0
36.07026 -3.51445 galactic Aql Second-epoch detections are separated by 1.1" 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 | ATO J287.4221+01.1782 | 19:09:40.52 +01:11:03.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:40.50 +01:11:06.0: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:40.50 +01:11:06.0: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.4221+01.1782,2461186.7012,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.4221+01.1782 20260526.2012 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.90 19:15:23.96 +03:00:51.4
38.35704 -3.94356 galactic Aql Second-epoch detections are separated by 2.4" and 1.6 pix
The object was found in VSX 4" Gaia DR3 4268193608109797760
Type: L
# Max. Min./Amp. JD0 Period
15.760 G 15.870 G
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:23.96 +03:00:51.4: 11.82 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:23.96 +03:00:51.4: 11.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4268193608109797760,2461186.7012,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268193608109797760 20260526.2012 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.06 19:12:03.17 +01:14:11.7
36.38927 -4.01898 galactic Aql Second-epoch detections are separated by 1.1" and 1.9 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 J288.0160+01.2327 | 19:12:03.22 +01:14:08.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.864+/-0.056 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:03.17 +01:14:11.7: 11.98 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:03.17 +01:14:11.7: 12.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.0160+01.2327,2461186.7012,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.0160+01.2327 20260526.2012 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.96 19:12:06.38 +01:35:19.2
36.70899 -3.86929 galactic Aql Second-epoch detections are separated by 0.8" 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 | Gaia DR3 4267796203365402496 | 19:12:06.45 +01:35:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.233+/-0.030 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:06.38 +01:35:19.2: 11.95 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:06.38 +01:35:19.2: 12.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267796203365402496,2461186.7012,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267796203365402496 20260526.2012 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.96 19:15:06.08 +02:06:40.6
37.51918 -4.29365 galactic Aql Second-epoch detections are separated by 2.5" and 2.4 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 4267887325388340736 | 19:15:06.10 +02:06:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.047+/-0.044 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:06.08 +02:06:40.6: 11.95 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:06.08 +02:06:40.6: 12.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267887325388340736,2461186.7012,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267887325388340736 20260526.2012 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.73 19:11:13.06 +00:53:34.5
35.98716 -3.99103 galactic Aql Second-epoch detections are separated by 1.8" and 2.1 pix
The object was found in VSX 5" ASASSN-V J191113.23+005330.9
Type: SR
# Max. Min./Amp. JD0 Period
13.500 g Y 0.280 g 2459529.55800 454.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:13.06 +00:53:34.5: 11.94 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:13.06 +00:53:34.5: 11.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191113.23+005330.9,2461186.7012,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191113.23+005330.9 20260526.2012 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.73 19:12:22.67 +01:00:55.9
36.22969 -4.19256 galactic Aql Second-epoch detections are separated by 0.6" and 2.0 pix
The object was found in VSX 3" ASASSN-V J191222.81+010053.3
Type: SR
# Max. Min./Amp. JD0 Period
13.920 g Y 0.320 g 2458667.71000 30.080000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:22.67 +01:00:55.9: 11.94 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:22.67 +01:00:55.9: 12.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191222.81+010053.3,2461186.7012,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191222.81+010053.3 20260526.2012 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.59 19:11:44.59 +01:09:26.4
36.28309 -3.98655 galactic Aql Second-epoch detections are separated by 0.5" and 2.1 pix
The object was found in VSX 3" ZTF J191144.70+010923.6
Type: SR
# Max. Min./Amp. JD0 Period
14.061 g Y 0.301 g 2458317.67740 125.252369200000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:44.59 +01:09:26.4: 11.93 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:44.59 +01:09:26.4: 12.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191144.70+010923.6,2461186.7012,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191144.70+010923.6 20260526.2012 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.89 19:10:45.87 +01:14:45.1
36.24953 -3.72858 galactic Aql Second-epoch detections are separated by 3.0" and 1.7 pix
The object was found in VSX17" ZTF J191045.42+011429.6
Type: RS
# Max. Min./Amp. JD0 Period
15.928 r Y 0.075 r 2458384.89510 16.831025900000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:45.87 +01:14:45.1: 11.93 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:45.87 +01:14:45.1: 11.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191045.42+011429.6,2461186.7012,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191045.42+011429.6 20260526.2012 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.97 18:30:48.38 +08:01:23.0
37.77872 8.21395 galactic Oph Second-epoch detections are separated by 0.8" and 2.0 pix
The object was found in VSX 0" ASASSN-V J183048.35+080123.1
Type: SRS
# Max. Min./Amp. JD0 Period
12.100 V 12.340 V 2457318.69300 28.760000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:30:48.38 +08:01:23.0: 11.90 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:30:48.38 +08:01:23.0: 11.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J183048.35+080123.1,2461186.7012,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183048.35+080123.1 20260526.2012 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.53 19:18:53.87 +04:17:35.9
39.89857 -4.12575 galactic Aql Second-epoch detections are separated by 1.6" and 1.9 pix
The object was found in VSX 4" V0812 Aql
Type: SR:
# Max. Min./Amp. JD0 Period
14.800 pg 16.800 pg 2426925.00000 150.000000000000 : M7-M8
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:18:53.87 +04:17:35.9: 11.88 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:18:53.87 +04:17:35.9: 11.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0812 Aql,2461186.7012,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0812 Aql 20260526.2012 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.89 19:21:45.03 +05:34:08.4
41.36217 -4.16135 galactic Aql Second-epoch detections are separated by 1.1" and 1.8 pix
The object was found in VSX 4" ASASSN-V J192145.28+053407.8
Type: SR
# Max. Min./Amp. JD0 Period
12.690 V 12.820 V 2458034.79100 46.280000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:21:45.03 +05:34:08.4: 11.88 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:21:45.03 +05:34:08.4: 11.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192145.28+053407.8,2461186.7012,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192145.28+053407.8 20260526.2012 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.38 19:16:44.49 +02:32:42.0
38.09458 -4.45739 galactic Aql Second-epoch detections are separated by 2.1" and 2.0 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 4267931786892660224 | 19:16:44.47 +02:32:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:44.49 +02:32:42.0: 12.48 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:44.49 +02:32:42.0: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267931786892660224,2461186.7012,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267931786892660224 20260526.2012 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 05 26.2012 2461186.7012 11.22 18:37:19.86 +07:47:43.9
38.30029 6.66649 galactic Oph Second-epoch detections are separated by 3.8" and 1.6 pix
The object was found in VSX 3" ASAS J183720+0747.7
Type: MISC
# Max. Min./Amp. JD0 Period
9.171 Ic Y 0.474 Ic 2453117.90000 209.010000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:37:19.86 +07:47:43.9: 12.28 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:37:19.86 +07:47:43.9: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183720+0747.7,2461186.7012,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J183720+0747.7 20260526.2012 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.76 19:21:37.63 +05:20:33.3
41.14699 -4.23978 galactic Aql Second-epoch detections are separated by 0.7" and 1.9 pix
The object was found in VSX 4" ASASSN-V J192137.90+052032.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.970 g Y 0.290 g 2459281.89100 28.438000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:21:37.63 +05:20:33.3: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:21:37.63 +05:20:33.3: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192137.90+052032.8,2461186.7012,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192137.90+052032.8 20260526.2012 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.34 18:35:40.81 +08:58:00.1
39.17306 7.55435 galactic Oph Second-epoch detections are separated by 2.0" and 1.9 pix
The object was found in VSX 1" ASASSN-V J183540.79+085759.6
Type: SRS
# Max. Min./Amp. JD0 Period
12.560 V 12.770 V 2457079.11900 28.907000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:35:40.81 +08:58:00.1: 12.38 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:35:40.81 +08:58:00.1: 12.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J183540.79+085759.6,2461186.7012,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183540.79+085759.6 20260526.2012 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 05 26.2012 2461186.7012 11.31 19:17:25.72 +03:04:12.4
38.64122 -4.36717 galactic Aql Second-epoch detections are separated by 2.7" 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 4292028133960343936 | 19:17:25.96 +03:04:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:25.72 +03:04:12.4: 12.41 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:25.72 +03:04:12.4: 12.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4292028133960343936,2461186.7012,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4292028133960343936 20260526.2012 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.44 19:19:24.42 +03:36:24.1
39.34750 -4.55660 galactic Aql Second-epoch detections are separated by 2.3" 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 | Gaia DR3 4292165813424231040 | 19:19:24.45 +03:36:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.258+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:19:24.42 +03:36:24.1: 12.43 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:19:24.42 +03:36:24.1: 12.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4292165813424231040,2461186.7012,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4292165813424231040 20260526.2012 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.04 19:17:26.16 +03:19:46.5
38.87281 -4.24886 galactic Aql Second-epoch detections are separated by 3.0" and 1.7 pix
The object was found in VSX 5" ASASSN-V J191726.45+031943.9
Type: SR
# Max. Min./Amp. JD0 Period
13.180 V 13.410 V 2457320.73200 43.090000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:26.16 +03:19:46.5: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:26.16 +03:19:46.5: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191726.45+031943.9,2461186.7012,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191726.45+031943.9 20260526.2012 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.96 19:12:18.71 +02:33:26.4
37.59473 -3.46975 galactic Aql Second-epoch detections are separated by 1.0" and 1.9 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 4268069844324791040 | 19:12:18.90 +02:33:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:18.71 +02:33:26.4: 11.82 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:18.71 +02:33:26.4: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4268069844324791040,2461186.7012,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268069844324791040 20260526.2012 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.70 19:15:41.66 +02:12:58.8
37.68112 -4.37677 galactic Aql Second-epoch detections are separated by 2.4" and 2.4 pix
The object was found in VSX 3" ASASSN-V J191541.85+021257.0
Type: SR
# Max. Min./Amp. JD0 Period
12.360 V 12.460 V 2457504.09200 35.830000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:41.66 +02:12:58.8: 11.79 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:41.66 +02:12:58.8: 11.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191541.85+021257.0,2461186.7012,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191541.85+021257.0 20260526.2012 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 05 26.2012 2461186.7012 10.78 19:16:18.18 +03:24:06.6
38.80602 -3.96472 galactic Aql Second-epoch detections are separated by 2.0" and 1.8 pix
The object was found in VSX 2" ASASSN-V J191618.33+032406.0
Type: SR
# Max. Min./Amp. JD0 Period
12.560 V 12.670 V 2457484.05400 46.440000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:18.18 +03:24:06.6: 11.82 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:18.18 +03:24:06.6: 11.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191618.33+032406.0,2461186.7012,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191618.33+032406.0 20260526.2012 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.38 19:12:58.76 +01:51:37.3
37.05132 -3.93828 galactic Aql Second-epoch detections are separated by 3.8" 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 | ATO J288.2426+01.8491 | 19:12:58.70 +01:51:35.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.948+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:58.76 +01:51:37.3: 12.39 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:58.76 +01:51:37.3: 12.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.2426+01.8491,2461186.7012,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.2426+01.8491 20260526.2012 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 05 26.2012 2461186.7012 10.95 19:13:43.37 +01:24:35.7
36.73576 -4.31025 galactic Aql Second-epoch detections are separated by 4.3" and 1.3 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 4267733634275164928 | 19:13:43.59 +01:24:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:43.37 +01:24:35.7: 11.89 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:43.37 +01:24:35.7: 11.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267733634275164928,2461186.7012,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267733634275164928 20260526.2012 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.53 19:11:37.11 +01:14:14.0
36.33993 -3.92223 galactic Aql Second-epoch detections are separated by 0.9" and 2.2 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 J287.9083+01.2370 | 19:11:37.04 +01:14:11.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:37.11 +01:14:14.0: 12.70 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:37.11 +01:14:14.0: 12.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.9083+01.2370,2461186.7012,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.9083+01.2370 20260526.2012 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.88 18:37:51.03 +09:35:49.2
39.98256 7.35493 galactic Oph Second-epoch detections are separated by 1.1" and 1.9 pix
The object was found in VSX 0" ASAS J183751+0935.8
Type: MISC
# Max. Min./Amp. JD0 Period
12.050 V Y 0.620 V 2452821.60000 137.683380000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:37:51.03 +09:35:49.2: 11.80 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:37:51.03 +09:35:49.2: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183751+0935.8,2461186.7012,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J183751+0935.8 20260526.2012 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 05 26.2012 2461186.7012 11.45 19:12:54.83 +02:13:22.8
37.36656 -3.75704 galactic Aql Second-epoch detections are separated by 1.0" and 2.0 pix
The object was found in VSX13" ZTF J191254.37+021334.1
Type: EW
# Max. Min./Amp. JD0 Period
18.890 r Y 0.845 r 2458376.67510 0.287439800000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:54.83 +02:13:22.8: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:54.83 +02:13:22.8: 12.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191254.37+021334.1,2461186.7012,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191254.37+021334.1 20260526.2012 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.29 19:16:59.69 +03:40:16.1
39.12540 -3.99331 galactic Aql Second-epoch detections are separated by 2.4" and 1.9 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 J289.2490+03.6704 | 19:16:59.77 +03:40:13.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:59.69 +03:40:16.1: 12.33 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:59.69 +03:40:16.1: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.2490+03.6704,2461186.7012,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.2490+03.6704 20260526.2012 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 05 26.2012 2461186.7012 11.71 18:49:58.85 +10:41:08.6
42.30351 5.16991 galactic Aql Second-epoch detections are separated by 1.2" and 1.7 pix
The object was found in VSX 3" ASAS J184959+1041.1
Type: SR
# Max. Min./Amp. JD0 Period
12.800 V 13.900 V 2457133.00000 92.560000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:49:58.85 +10:41:08.6: 12.65 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:49:58.85 +10:41:08.6: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184959+1041.1,2461186.7012,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184959+1041.1 20260526.2012 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 05 26.2012 2461186.7012 11.48 19:16:34.08 +03:27:26.8
38.88609 -3.99767 galactic Aql Second-epoch detections are separated by 0.5" and 2.2 pix
The object was found in VSX 2" ASASSN-V J191634.20+032725.9
Type: SRS
# Max. Min./Amp. JD0 Period
13.510 V 13.630 V 2457112.12100 25.510000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:34.08 +03:27:26.8: 12.69 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:34.08 +03:27:26.8: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191634.20+032725.9,2461186.7012,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191634.20+032725.9 20260526.2012 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.90 18:34:56.38 +08:10:00.6
38.36857 7.36204 galactic Oph Second-epoch detections are separated by 2.1" and 1.5 pix
The object was found in VSX 2" NSVS 11097645
Type: SR
# Max. Min./Amp. JD0 Period
14.526 g Y 0.511 g 2458641.56760 511.909873000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:34:56.38 +08:10:00.6: 13.09 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:34:56.38 +08:10:00.6: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11097645,2461186.7012,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11097645 20260526.2012 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 05 26.2012 2461186.7012 11.63 18:30:20.44 +09:58:11.0
39.49297 9.17901 galactic Oph Second-epoch detections are separated by 2.6" and 2.2 pix
The object was found in VSX 0" ASASSN-V J183020.43+095810.7
Type: L
# Max. Min./Amp. JD0 Period
12.940 V 13.730 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:30:20.44 +09:58:11.0: 12.67 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:30:20.44 +09:58:11.0: 12.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J183020.43+095810.7,2461186.7012,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183020.43+095810.7 20260526.2012 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.24 19:09:25.59 +01:00:44.5
35.88800 -3.53832 galactic Aql Second-epoch detections are separated by 1.5" and 2.0 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 J287.3575+00.9991 | 19:09:25.76 +01:00:42.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:25.59 +01:00:44.5: 12.30 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:25.59 +01:00:44.5: 12.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.3575+00.9991,2461186.7012,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.3575+00.9991 20260526.2012 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.39 19:14:13.57 +02:11:10.8
37.48509 -4.06500 galactic Aql Second-epoch detections are separated by 1.2" and 1.9 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 4267939139876987136 | 19:14:13.60 +02:11:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:13.57 +02:11:10.8: 12.34 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:13.57 +02:11:10.8: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267939139876987136,2461186.7012,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267939139876987136 20260526.2012 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 05 26.2012 2461186.7012 11.12 19:12:33.70 +01:40:10.4
36.83338 -3.93323 galactic Aql Second-epoch detections are separated by 3.1" and 2.6 pix
The object was found in VSX 3" ASASSN-V J191233.74+014007.5
Type: SR
# Max. Min./Amp. JD0 Period
13.040 V 13.270 V 2457232.00000 535.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:33.70 +01:40:10.4: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:33.70 +01:40:10.4: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191233.74+014007.5,2461186.7012,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191233.74+014007.5 20260526.2012 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.14 19:15:33.78 +02:27:12.9
37.87712 -4.23835 galactic Aql Second-epoch detections are separated by 2.0" 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 | ATO J288.8983+02.4556 | 19:15:33.88 +02:27:10.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:33.78 +02:27:12.9: 12.33 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:33.78 +02:27:12.9: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.8983+02.4556,2461186.7012,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.8983+02.4556 20260526.2012 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.36 19:19:09.82 +03:22:01.2
39.10617 -4.61381 galactic Aql Second-epoch detections are separated by 1.9" and 2.3 pix
The object was found in VSX 3" ASASSN-V J191910.01+032159.8
Type: L
# Max. Min./Amp. JD0 Period
12.950 V 13.060 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:19:09.82 +03:22:01.2: 12.33 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:19:09.82 +03:22:01.2: 12.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191910.01+032159.8,2461186.7012,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191910.01+032159.8 20260526.2012 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 05 26.2012 2461186.7012 11.34 19:15:31.50 +02:08:35.3
37.59642 -4.37294 galactic Aql Second-epoch detections are separated by 1.7" and 2.1 pix
The object was found in VSX23" Gaia DR3 4267886260190566144
Type:
# Max. Min./Amp. JD0 Period
19.250 G 19.430 G 0.483029000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:31.50 +02:08:35.3: 12.35 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:31.50 +02:08:35.3: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267886260190566144,2461186.7012,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267886260190566144 20260526.2012 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 05 26.2012 2461186.7012 11.34 18:34:15.36 +09:04:11.0
39.10851 7.91514 galactic Oph Second-epoch detections are separated by 1.2" and 1.7 pix
The object was found in VSX 1" V0624 Oph
Type: SR
# Max. Min./Amp. JD0 Period
13.600 pg 14.600 pg 2425781.00000 182.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:34:15.36 +09:04:11.0: 12.66 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:34:15.36 +09:04:11.0: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0624 Oph,2461186.7012,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0624 Oph 20260526.2012 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 05 26.2012 2461186.7012 11.51 19:10:43.80 +01:16:32.7
36.27218 -3.70721 galactic Aql Second-epoch detections are separated by 1.0" 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 J287.6717+01.2730 | 19:10:43.86 +01:16:29.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:43.80 +01:16:32.7: 12.50 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:43.80 +01:16:32.7: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.6717+01.2730,2461186.7012,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.6717+01.2730 20260526.2012 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 05 26.2012 2461186.7012 11.28 19:12:05.39 +02:21:10.6
37.38735 -3.51450 galactic Aql Second-epoch detections are separated by 1.9" and 1.9 pix
The object was found in VSX 2" ASASSN-V J191205.29+022110.6
Type: SRS
# Max. Min./Amp. JD0 Period
13.000 V 13.100 V 2457600.93800 24.640000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:05.39 +02:21:10.6: 12.31 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:05.39 +02:21:10.6: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191205.29+022110.6,2461186.7012,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191205.29+022110.6 20260526.2012 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.36 19:13:42.31 +01:59:41.7
37.25468 -4.03748 galactic Aql Second-epoch detections are separated by 3.5" and 2.0 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 J288.4168+01.9919 | 19:13:42.33 +01:59:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.747+/-0.032 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:42.31 +01:59:41.7: 12.29 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:42.31 +01:59:41.7: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.4168+01.9919,2461186.7012,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.4168+01.9919 20260526.2012 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 05 26.2012 2461186.7012 11.66 19:08:42.78 +01:22:46.1
36.13306 -3.21163 galactic Aql Second-epoch detections are separated by 2.3" and 2.4 pix
The object was found in VSX 4" ASASSN-V J190842.91+012243.1
Type: L
# Max. Min./Amp. JD0 Period
13.860 V 14.430 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:42.78 +01:22:46.1: 12.91 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:42.78 +01:22:46.1: 12.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190842.91+012243.1,2461186.7012,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190842.91+012243.1 20260526.2012 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.79 19:13:23.64 +01:52:46.4
37.11614 -4.02148 galactic Aql Second-epoch detections are separated by 1.2" 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 J288.3391+01.8731 | 19:13:20.84 +01:52:44.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.796+/-0.031 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:23.64 +01:52:46.4: 11.73 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:23.64 +01:52:46.4: 11.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.3391+01.8731,2461186.7012,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.3391+01.8731 20260526.2012 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 05 26.2012 2461186.7012 10.80 19:12:48.43 +01:45:53.5
36.94648 -3.94395 galactic Aql Second-epoch detections are separated by 0.8" and 2.2 pix
The object was found in VSX19" Gaia DR3 4267805377413948288
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.040 G 13.060 G B
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:48.43 +01:45:53.5: 11.66 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:48.43 +01:45:53.5: 11.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267805377413948288,2461186.7012,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267805377413948288 20260526.2012 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 05 26.2012 2461186.7012 10.71 19:16:17.63 +02:19:17.0
37.84384 -4.46128 galactic Aql Second-epoch detections are separated by 2.5" and 2.4 pix
The object was found in VSX 4" ASASSN-V J191617.81+021914.6
Type: SRS
# Max. Min./Amp. JD0 Period
13.330 g Y 0.220 g 2458673.51700 29.450000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:17.63 +02:19:17.0: 11.70 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:17.63 +02:19:17.0: 11.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191617.81+021914.6,2461186.7012,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191617.81+021914.6 20260526.2012 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.50 19:12:22.99 +01:07:09.0
36.32264 -4.14621 galactic Aql Second-epoch detections are separated by 0.9" and 2.0 pix
The object was found in VSX20" Gaia DR3 4267346636206444032
Type: YSO
# Max. Min./Amp. JD0 Period
17.350 G 17.470 G M
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:22.99 +01:07:09.0: 12.64 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:22.99 +01:07:09.0: 12.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267346636206444032,2461186.7012,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267346636206444032 20260526.2012 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.19 19:15:05.00 +03:03:55.6
38.36607 -3.84996 galactic Aql Second-epoch detections are separated by 1.5" and 2.0 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 J288.7646+03.0583 | 19:15:05.07 +03:03:55.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.306+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:05.00 +03:03:55.6: 12.30 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:05.00 +03:03:55.6: 12.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.7646+03.0583,2461186.7012,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.7646+03.0583 20260526.2012 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.24 19:19:09.96 +03:21:17.4
39.09562 -4.61996 galactic Aql Second-epoch detections are separated by 0.7" and 2.1 pix
The object was found in VSX 3" ASASSN-V J191910.15+032115.6
Type: SR
# Max. Min./Amp. JD0 Period
13.150 V 13.330 V 2457509.06700 41.230000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:19:09.96 +03:21:17.4: 12.28 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:19:09.96 +03:21:17.4: 12.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191910.15+032115.6,2461186.7012,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191910.15+032115.6 20260526.2012 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.74 19:15:17.09 +02:11:14.3
37.60803 -4.29934 galactic Aql Second-epoch detections are separated by 2.5" 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 J288.8278+02.1800 | 19:15:17.17 +02:11:12.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.175+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:17.09 +02:11:14.3: 11.69 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:17.09 +02:11:14.3: 11.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.8278+02.1800,2461186.7012,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.8278+02.1800 20260526.2012 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.73 19:12:38.61 +00:58:49.9
36.22904 -4.26762 galactic Aql Second-epoch detections are separated by 2.3" and 1.9 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 J288.1686+00.9860 | 19:12:38.57 +00:58:47.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.692+/-0.031 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:38.61 +00:58:49.9: 11.64 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:38.61 +00:58:49.9: 11.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.1686+00.9860,2461186.7012,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.1686+00.9860 20260526.2012 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.57 19:13:49.37 +02:21:19.6
37.58911 -3.89772 galactic Aql Second-epoch detections are separated by 1.1" and 2.2 pix
The object was found in VSX 2" ASASSN-V J191349.44+022117.7
Type: SR
# Max. Min./Amp. JD0 Period
12.260 V 12.370 V 2458308.99200 33.340000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:49.37 +02:21:19.6: 11.68 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:49.37 +02:21:19.6: 11.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191349.44+022117.7,2461186.7012,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191349.44+022117.7 20260526.2012 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 05 26.2012 2461186.7012 11.53 19:12:04.74 +01:07:02.9
36.28617 -4.07943 galactic Aql Second-epoch detections are separated by 0.7" and 2.0 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 J288.0209+01.1165 | 19:12:05.02 +01:06:59.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:04.74 +01:07:02.9: 12.89 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:04.74 +01:07:02.9: 12.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.0209+01.1165,2461186.7012,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.0209+01.1165 20260526.2012 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.41 19:18:32.77 +03:33:36.4
39.20630 -4.38782 galactic Aql Second-epoch detections are separated by 2.2" and 2.0 pix
The object was found in VSX 4" ASASSN-V J191833.07+033335.7
Type: SR
# Max. Min./Amp. JD0 Period
13.770 V 13.930 V 2457977.92100 40.880000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:18:32.77 +03:33:36.4: 12.89 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:18:32.77 +03:33:36.4: 13.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191833.07+033335.7,2461186.7012,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191833.07+033335.7 20260526.2012 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 05 26.2012 2461186.7012 11.59 19:19:05.82 +03:33:07.7
39.26305 -4.51333 galactic Aql Second-epoch detections are separated by 1.5" and 2.4 pix
The object was found in VSX 5" ASASSN-V J191906.12+033306.6
Type: SR
# Max. Min./Amp. JD0 Period
14.370 V 15.060 V 2458322.71020 156.286195000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:19:05.82 +03:33:07.7: 13.07 +/- 0.05 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:19:05.82 +03:33:07.7: 13.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191906.12+033306.6,2461186.7012,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191906.12+033306.6 20260526.2012 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 05 26.2012 2461186.7012 11.63 19:09:15.41 +01:05:04.1
35.93277 -3.46760 galactic Aql Second-epoch detections are separated by 4.0" and 1.6 pix
The object was found in VSX 4" ASASSN-V J190915.56+010500.6
Type: SRS
# Max. Min./Amp. JD0 Period
13.730 V 13.890 V 2457083.12000 24.909000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:15.41 +01:05:04.1: 12.88 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:15.41 +01:05:04.1: 12.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190915.56+010500.6,2461186.7012,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190915.56+010500.6 20260526.2012 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.66 19:20:58.87 +03:59:47.1
39.87664 -4.72368 galactic Aql Second-epoch detections are separated by 0.5" and 2.0 pix
The object was found in VSX 2" ASASSN-V J192058.99+035945.9
Type: SR
# Max. Min./Amp. JD0 Period
13.400 g Y 0.370 g 2459338.79400 30.840000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:20:58.87 +03:59:47.1: 11.68 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:20:58.87 +03:59:47.1: 11.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192058.99+035945.9,2461186.7012,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192058.99+035945.9 20260526.2012 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.54 19:14:42.73 +02:51:60.0
38.14645 -3.85939 galactic Aql Second-epoch detections are separated by 2.7" and 2.4 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 J288.6783+02.8702 | 19:14:42.70 +02:51:59.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.945+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:42.73 +02:51:60.0: 12.62 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:42.73 +02:51:60.0: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.6783+02.8702,2461186.7012,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6783+02.8702 20260526.2012 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 05 26.2012 2461186.7012 11.16 19:15:07.67 +02:21:22.9
37.74039 -4.18667 galactic Aql Second-epoch detections are separated by 0.9" and 1.8 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 4267945462069476224 | 19:15:10.40 +02:21:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+02 2405
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:07.67 +02:21:22.9: 12.34 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:07.67 +02:21:22.9: 12.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267945462069476224,2461186.7012,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267945462069476224 20260526.2012 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 05 26.2012 2461186.7012 11.18 19:15:20.01 +02:31:03.6
37.90766 -4.15795 galactic Aql Second-epoch detections are separated by 1.3" and 2.0 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 J288.8353+02.5196 | 19:15:20.01 +02:31:00.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:20.01 +02:31:03.6: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:20.01 +02:31:03.6: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.8353+02.5196,2461186.7012,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.8353+02.5196 20260526.2012 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 05 26.2012 2461186.7012 11.28 19:12:20.36 +01:55:15.4
37.03161 -3.76841 galactic Aql Second-epoch detections are separated by 1.2" and 2.2 pix
The object was found in VSX13" Gaia DR3 4267811493447939456
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.720 G 14.750 G A
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:20.36 +01:55:15.4: 12.28 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:20.36 +01:55:15.4: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267811493447939456,2461186.7012,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267811493447939456 20260526.2012 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.25 19:14:21.38 +03:10:09.9
38.37464 -3.64098 galactic Aql Second-epoch detections are separated by 0.6" and 2.0 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 4268212849564841856 | 19:14:21.50 +03:10:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:21.38 +03:10:09.9: 12.25 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:21.38 +03:10:09.9: 12.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4268212849564841856,2461186.7012,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268212849564841856 20260526.2012 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.76 18:36:44.34 +09:00:04.4
39.32156 7.33555 galactic Oph Second-epoch detections are separated by 1.5" and 1.7 pix
The object was found in VSX 2" V0638 Oph
Type: L
# Max. Min./Amp. JD0 Period
15.100 pg 15.800 pg
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:36:44.34 +09:00:04.4: 13.08 +/- 0.05 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:36:44.34 +09:00:04.4: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0638 Oph,2461186.7012,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0638 Oph 20260526.2012 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 05 26.2012 2461186.7012 11.60 18:35:59.12 +09:27:39.2
39.65351 7.70647 galactic Oph Second-epoch detections are separated by 0.6" and 1.8 pix
The object was found in VSX 1" ASAS J183600+0927.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.780 V Y 0.400 V 2452256.90000 29.224230000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:35:59.12 +09:27:39.2: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:35:59.12 +09:27:39.2: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183600+0927.7,2461186.7012,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J183600+0927.7 20260526.2012 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 05 26.2012 2461186.7012 11.52 19:14:06.44 +01:50:04.1
37.15816 -4.20049 galactic Aql Second-epoch detections are separated by 1.7" and 2.4 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 J288.5270+01.8339 | 19:14:06.50 +01:50:02.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.355+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:06.44 +01:50:04.1: 12.87 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:06.44 +01:50:04.1: 12.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.5270+01.8339,2461186.7012,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.5270+01.8339 20260526.2012 11.52CV 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 05 26.2012 2461186.7012 11.15 19:22:17.57 +05:43:17.0
41.56045 -4.20957 galactic Aql Second-epoch detections are separated by 0.8" and 2.0 pix
The object was found in VSX 5" ASASSN-V J192217.89+054318.2
Type: SR
# Max. Min./Amp. JD0 Period
14.360 g Y 0.460 g 2458292.73400 313.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:22:17.57 +05:43:17.0: 12.23 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:22:17.57 +05:43:17.0: 12.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192217.89+054318.2,2461186.7012,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192217.89+054318.2 20260526.2012 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 05 26.2012 2461186.7012 11.17 19:12:47.48 +01:23:15.5
36.60874 -4.11366 galactic Aql Second-epoch detections are separated by 1.5" and 2.0 pix
The object was found in VSX 3" ZTF J191247.66+012314.3
Type: SR
# Max. Min./Amp. JD0 Period
14.747 g Y 0.482 g 2458649.32700 243.910037200000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:47.48 +01:23:15.5: 12.55 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:47.48 +01:23:15.5: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191247.66+012314.3,2461186.7012,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191247.66+012314.3 20260526.2012 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.23 19:16:31.51 +03:23:26.8
38.82188 -4.01900 galactic Aql Second-epoch detections are separated by 0.4" 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 J289.1334+03.3804 | 19:16:31.59 +03:23:24.9 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.231+/-0.037 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:31.51 +03:23:26.8: 12.24 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:31.51 +03:23:26.8: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.1334+03.3804,2461186.7012,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.1334+03.3804 20260526.2012 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 05 26.2012 2461186.7012 11.29 19:16:28.64 +02:56:23.9
38.41546 -4.21661 galactic Aql Second-epoch detections are separated by 1.6" and 2.0 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 4292020025061652992 | 19:16:28.75 +02:56:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.031 (G)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:28.64 +02:56:23.9: 12.23 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:28.64 +02:56:23.9: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4292020025061652992,2461186.7012,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4292020025061652992 20260526.2012 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 05 26.2012 2461186.7012 11.31 19:11:33.77 +01:05:12.0
36.19942 -3.97890 galactic Aql Second-epoch detections are separated by 1.0" and 1.9 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 J287.8909+01.0852 | 19:11:33.82 +01:05:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:33.77 +01:05:12.0: 12.57 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:33.77 +01:05:12.0: 12.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.8909+01.0852,2461186.7012,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.8909+01.0852 20260526.2012 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.64 18:36:18.15 +08:04:10.9
38.43266 7.01684 galactic Oph Second-epoch detections are separated by 2.8" and 2.4 pix
The object was found in VSX 1" ASAS J183618+0804.2
Type: MISC
# Max. Min./Amp. JD0 Period
9.164 Ic Y 0.200 Ic 2452499.80000 39.590000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:36:18.15 +08:04:10.9: 12.84 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:36:18.15 +08:04:10.9: 12.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183618+0804.2,2461186.7012,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J183618+0804.2 20260526.2012 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 05 26.2012 2461186.7012 11.26 19:21:48.79 +05:07:49.7
40.98044 -4.37961 galactic Aql Second-epoch detections are separated by 0.8" 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 J290.4536+05.1301 | 19:21:48.86 +05:07:48.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.834+/-0.035 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:21:48.79 +05:07:49.7: 12.23 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:21:48.79 +05:07:49.7: 12.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J290.4536+05.1301,2461186.7012,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J290.4536+05.1301 20260526.2012 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.30 19:15:29.29 +02:19:06.1
37.74814 -4.28406 galactic Aql Second-epoch detections are separated by 1.0" and 2.1 pix
The object was found in VSX 4" ASAS J191529+0219.0
Type: MISC
# Max. Min./Amp. JD0 Period
13.070 V Y 0.380 V 2452275.10000 52.110390000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:29.29 +02:19:06.1: 11.61 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:29.29 +02:19:06.1: 11.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191529+0219.0,2461186.7012,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J191529+0219.0 20260526.2012 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.29 19:15:59.79 +02:11:07.1
37.68837 -4.45807 galactic Aql Second-epoch detections are separated by 1.8" and 2.2 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 4267892410629944064 | 19:15:59.91 +02:11:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:59.79 +02:11:07.1: 12.22 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:59.79 +02:11:07.1: 12.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267892410629944064,2461186.7012,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267892410629944064 20260526.2012 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 05 26.2012 2461186.7012 11.14 19:09:58.61 +01:40:52.7
36.54678 -3.35396 galactic Aql Second-epoch detections are separated by 2.5" and 1.7 pix
The object was found in VSX 4" ASASSN-V J190958.83+014050.0
Type: L
# Max. Min./Amp. JD0 Period
12.830 V 12.990 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:58.61 +01:40:52.7: 12.23 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:58.61 +01:40:52.7: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190958.83+014050.0,2461186.7012,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190958.83+014050.0 20260526.2012 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.32 19:16:43.76 +02:53:56.7
38.40822 -4.29130 galactic Aql Second-epoch detections are separated by 2.8" and 1.8 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 J289.1857+02.8916 | 19:16:43.90 +02:53:56.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.214+/-0.048 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:43.76 +02:53:56.7: 12.57 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:43.76 +02:53:56.7: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.1857+02.8916,2461186.7012,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.1857+02.8916 20260526.2012 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 05 26.2012 2461186.7012 11.58 19:12:24.66 +01:12:47.1
36.40951 -4.10931 galactic Aql Second-epoch detections are separated by 1.7" and 2.2 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 4267352030680844032 | 19:12:24.79 +01:12:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.334+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:24.66 +01:12:47.1: 12.82 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:24.66 +01:12:47.1: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267352030680844032,2461186.7012,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267352030680844032 20260526.2012 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.46 19:11:25.00 +01:44:06.8
36.76018 -3.64890 galactic Aql Second-epoch detections are separated by 1.9" and 2.4 pix
The object was found in VSX 6" ASASSN-V J191125.18+014401.1
Type: SR
# Max. Min./Amp. JD0 Period
14.210 g Y 0.190 g 2459476.37500 527.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:25.00 +01:44:06.8: 12.52 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:25.00 +01:44:06.8: 12.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191125.18+014401.1,2461186.7012,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191125.18+014401.1 20260526.2012 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 05 26.2012 2461186.7012 10.35 19:14:28.31 +02:02:54.2
37.39061 -4.18296 galactic Aql Second-epoch detections are separated by 1.7" and 1.8 pix
The object was found in VSX 3" ASASSN-V J191428.43+020251.8
Type: SR
# Max. Min./Amp. JD0 Period
13.160 g Y 0.260 g 2459374.85900 30.930000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:28.31 +02:02:54.2: 11.56 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:28.31 +02:02:54.2: 11.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191428.43+020251.8,2461186.7012,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191428.43+020251.8 20260526.2012 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.60 19:17:59.56 +03:41:43.2
39.26239 -4.20281 galactic Aql Second-epoch detections are separated by 0.6" 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 J289.5064+03.6965 | 19:17:59.67 +03:41:42.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.326+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:59.56 +03:41:43.2: 11.56 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:59.56 +03:41:43.2: 11.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.5064+03.6965,2461186.7012,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.5064+03.6965 20260526.2012 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.21 19:15:59.29 +03:28:20.5
38.83234 -3.86246 galactic Aql Second-epoch detections are separated by 1.1" and 2.0 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 4292245115714450560 | 19:15:59.30 +03:28:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:59.29 +03:28:20.5: 12.21 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:59.29 +03:28:20.5: 12.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4292245115714450560,2461186.7012,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4292245115714450560 20260526.2012 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 05 26.2012 2461186.7012 11.14 19:20:54.22 +04:24:59.7
40.24091 -4.51134 galactic Aql Second-epoch detections are separated by 0.4" and 1.9 pix
The object was found in VSX 3" ASASSN-V J192054.38+042458.8
Type: SR
# Max. Min./Amp. JD0 Period
13.710 g Y 0.220 g 2459499.33000 506.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:20:54.22 +04:24:59.7: 12.21 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:20:54.22 +04:24:59.7: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192054.38+042458.8,2461186.7012,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192054.38+042458.8 20260526.2012 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.26 19:19:11.82 +03:42:32.2
39.41404 -4.46279 galactic Aql Second-epoch detections are separated by 3.2" and 1.9 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 J289.7994+03.7087 | 19:19:11.86 +03:42:31.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.810+/-0.029 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:19:11.82 +03:42:32.2: 12.21 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:19:11.82 +03:42:32.2: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.7994+03.7087,2461186.7012,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.7994+03.7087 20260526.2012 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.25 19:10:34.26 +00:53:03.3
35.90521 -3.85131 galactic Aql Second-epoch detections are separated by 1.9" and 2.5 pix
The object was found in VSX15" Gaia DR3 4267315815542683008
Type: RS
# Max. Min./Amp. JD0 Period
17.210 G 17.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:34.26 +00:53:03.3: 12.21 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:34.26 +00:53:03.3: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267315815542683008,2461186.7012,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267315815542683008 20260526.2012 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.07 19:15:35.37 +02:44:04.2
38.13014 -4.11473 galactic Aql Second-epoch detections are separated by 0.9" 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 J288.8919+02.7247 | 19:15:35.56 +02:44:08.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:35.37 +02:44:04.2: 12.20 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:35.37 +02:44:04.2: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.8919+02.7247,2461186.7012,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.8919+02.7247 20260526.2012 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.23 19:15:54.53 +02:44:55.9
38.17978 -4.17886 galactic Aql Second-epoch detections are separated by 1.4" and 2.0 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 J288.9778+02.7602 | 19:15:54.58 +02:44:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.723+/-0.033 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:54.53 +02:44:55.9: 12.18 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:54.53 +02:44:55.9: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.9778+02.7602,2461186.7012,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.9778+02.7602 20260526.2012 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 05 26.2012 2461186.7012 10.63 19:09:22.42 +01:12:15.4
36.05286 -3.43867 galactic Aql Second-epoch detections are separated by 0.7" and 2.0 pix
The object was found in VSX 3" ASASSN-V J190922.57+011213.0
Type: SR
# Max. Min./Amp. JD0 Period
13.360 g Y 0.290 g 2458703.48800 454.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:22.42 +01:12:15.4: 11.51 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:22.42 +01:12:15.4: 11.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190922.57+011213.0,2461186.7012,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190922.57+011213.0 20260526.2012 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.57 18:37:18.07 +09:11:21.6
39.55367 7.29499 galactic Oph Second-epoch detections are separated by 1.9" and 1.6 pix
The object was found in VSX 2" V0641 Oph
Type: LB:
# Max. Min./Amp. JD0 Period
14.200 pg 15.400 pg M
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:37:18.07 +09:11:21.6: 12.81 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:37:18.07 +09:11:21.6: 12.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0641 Oph,2461186.7012,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0641 Oph 20260526.2012 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 05 26.2012 2461186.7012 11.74 18:38:25.02 +08:58:31.5
39.48429 6.95308 galactic Oph Second-epoch detections are separated by 1.2" and 1.8 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 4479477171215294208 | 18:38:25.06 +08:58:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.237+/-0.032 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:38:25.02 +08:58:31.5: 12.81 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:38:25.02 +08:58:31.5: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4479477171215294208,2461186.7012,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4479477171215294208 20260526.2012 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.55 19:12:45.60 +01:33:22.1
36.75520 -4.02934 galactic Aql Second-epoch detections are separated by 0.3" 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 | Gaia DR3 4267745557105118080 | 19:12:45.67 +01:33:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.203+/-0.035 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:45.60 +01:33:22.1: 11.50 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:45.60 +01:33:22.1: 11.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267745557105118080,2461186.7012,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267745557105118080 20260526.2012 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.19 19:09:52.82 +01:08:27.6
36.05464 -3.58023 galactic Aql Second-epoch detections are separated by 2.6" 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 4267383023181527168 | 19:09:52.90 +01:08:28.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.807+/-0.033 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:52.82 +01:08:27.6: 12.19 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:52.82 +01:08:27.6: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267383023181527168,2461186.7012,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267383023181527168 20260526.2012 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.95 19:17:00.90 +03:03:21.5
38.58079 -4.28211 galactic Aql Second-epoch detections are separated by 1.8" and 2.0 pix
The object was found in VSX 5" ASASSN-V J191701.16+030318.9
Type: SR
# Max. Min./Amp. JD0 Period
13.160 V 13.300 V 2457113.07300 51.710000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:00.90 +03:03:21.5: 12.20 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:00.90 +03:03:21.5: 12.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191701.16+030318.9,2461186.7012,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191701.16+030318.9 20260526.2012 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.24 19:17:03.27 +03:16:34.1
38.78116 -4.18913 galactic Aql Second-epoch detections are separated by 5.7" 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 J289.2581+03.2782 | 19:17:03.80 +03:16:31.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:03.27 +03:16:34.1: 12.13 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:03.27 +03:16:34.1: 12.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.2581+03.2782,2461186.7012,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.2581+03.2782 20260526.2012 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.94 19:17:17.99 +03:18:40.6
38.84078 -4.22719 galactic Aql Second-epoch detections are separated by 0.3" and 2.3 pix
The object was found in VSX 3" ASASSN-V J191718.21+031839.8
Type: SR
# Max. Min./Amp. JD0 Period
13.110 V 13.370 V 2457697.00000 503.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:17.99 +03:18:40.6: 12.19 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:17.99 +03:18:40.6: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191718.21+031839.8,2461186.7012,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191718.21+031839.8 20260526.2012 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.53 19:11:04.68 +01:56:12.2
36.90061 -3.48121 galactic Aql Second-epoch detections are separated by 0.7" 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 J287.7609+01.9414 | 19:11:04.75 +01:56:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:04.68 +01:56:12.2: 12.54 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:04.68 +01:56:12.2: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.7609+01.9414,2461186.7012,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.7609+01.9414 20260526.2012 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.12 19:15:51.47 +01:41:49.2
37.23752 -4.65212 galactic Aql Second-epoch detections are separated by 2.1" and 2.2 pix
The object was found in VSX 4" NSVS 14045678
Type: L
# Max. Min./Amp. JD0 Period
10.600 R1 10.950 R1
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:51.47 +01:41:49.2: 12.18 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:51.47 +01:41:49.2: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 14045678,2461186.7012,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 14045678 20260526.2012 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.93 19:08:55.77 +00:54:57.0
35.74503 -3.47209 galactic Aql Second-epoch detections are separated by 2.3" and 1.8 pix
The object was found in VSX 5" ASASSN-V J190856.01+005454.1
Type: SR
# Max. Min./Amp. JD0 Period
12.920 V 13.080 V 2458260.00000 642.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:55.77 +00:54:57.0: 12.16 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:55.77 +00:54:57.0: 12.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190856.01+005454.1,2461186.7012,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190856.01+005454.1 20260526.2012 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 05 26.2012 2461186.7012 11.19 19:08:54.40 +01:19:41.5
36.10962 -3.27814 galactic Aql Second-epoch detections are separated by 2.6" and 1.8 pix
The object was found in VSX 3" ASASSN-V J190854.47+011938.9
Type: SRS
# Max. Min./Amp. JD0 Period
12.870 V 12.990 V 2457430.16700 21.945000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:54.40 +01:19:41.5: 12.17 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:54.40 +01:19:41.5: 12.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190854.47+011938.9,2461186.7012,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190854.47+011938.9 20260526.2012 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.26 19:16:09.46 +02:41:47.4
38.16194 -4.25814 galactic Aql Second-epoch detections are separated by 1.9" and 1.8 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 4267984391655494272 | 19:16:09.55 +02:41:43.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:09.46 +02:41:47.4: 12.16 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:09.46 +02:41:47.4: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267984391655494272,2461186.7012,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267984391655494272 20260526.2012 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.51 19:15:59.03 +03:42:28.9
39.04130 -3.75261 galactic Aql Second-epoch detections are separated by 1.0" and 2.0 pix
The object was found in VSX 3" ASASSN-V J191559.13+034226.4
Type: SRS
# Max. Min./Amp. JD0 Period
13.380 V 13.490 V 2457327.70900 20.573000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:59.03 +03:42:28.9: 12.56 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:59.03 +03:42:28.9: 12.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191559.13+034226.4,2461186.7012,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191559.13+034226.4 20260526.2012 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 05 26.2012 2461186.7012 10.96 19:09:49.48 +01:25:27.0
36.30040 -3.43808 galactic Aql Second-epoch detections are separated by 1.0" and 2.2 pix
The object was found in VSX 3" ZTF J190949.61+012524.9
Type: SR
# Max. Min./Amp. JD0 Period
14.023 g Y 0.194 g 2458379.30280 96.570618600000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:49.48 +01:25:27.0: 12.13 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:49.48 +01:25:27.0: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190949.61+012524.9,2461186.7012,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190949.61+012524.9 20260526.2012 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.56 18:22:48.75 +08:35:49.3
37.41223 10.24100 galactic Oph Second-epoch detections are separated by 2.4" and 1.5 pix
The object was found in VSX 1" ASASSN-V J182248.71+083548.0
Type: SR
# Max. Min./Amp. JD0 Period
12.940 V 13.150 V 2458304.00000 539.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:22:48.75 +08:35:49.3: 12.56 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:22:48.75 +08:35:49.3: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J182248.71+083548.0,2461186.7012,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182248.71+083548.0 20260526.2012 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 05 26.2012 2461186.7012 11.08 19:15:35.44 +02:49:51.5
38.21609 -4.07050 galactic Aql Second-epoch detections are separated by 2.0" and 1.6 pix
The object was found in VSX14" Gaia DR3 4268001193568708224
Type: RS
# Max. Min./Amp. JD0 Period
17.100 G 17.220 G
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:35.44 +02:49:51.5: 12.17 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:35.44 +02:49:51.5: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4268001193568708224,2461186.7012,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268001193568708224 20260526.2012 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 05 26.2012 2461186.7012 11.54 19:17:08.71 +02:53:14.9
38.44596 -4.38876 galactic Aql Second-epoch detections are separated by 5.6" and 3.0 pix
The object was found in VSX 5" ASASSN-V J191709.05+025313.4
Type: SR
# Max. Min./Amp. JD0 Period
14.270 V 14.550 V 2458235.93180 38.396215000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:08.71 +02:53:14.9: 13.01 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:08.71 +02:53:14.9: 13.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191709.05+025313.4,2461186.7012,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191709.05+025313.4 20260526.2012 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 05 26.2012 2461186.7012 11.49 18:29:40.19 +07:38:22.2
37.30505 8.29526 galactic Oph Second-epoch detections are separated by 1.6" and 1.6 pix
The object was found in VSX 2" ASASSN-V J182940.16+073820.0
Type: SR
# Max. Min./Amp. JD0 Period
12.690 V 12.950 V 2457431.20000 45.690000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:29:40.19 +07:38:22.2: 12.52 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:29:40.19 +07:38:22.2: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J182940.16+073820.0,2461186.7012,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182940.16+073820.0 20260526.2012 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.52 19:12:41.25 +02:15:06.7
37.36619 -3.69356 galactic Aql Second-epoch detections are separated by 2.4" and 1.9 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 4267861280712702848 | 19:12:41.23 +02:15:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:41.25 +02:15:06.7: 12.47 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:41.25 +02:15:06.7: 12.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267861280712702848,2461186.7012,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267861280712702848 20260526.2012 11.52CV 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 05 26.2012 2461186.7012 11.46 19:16:24.58 +02:44:49.4
38.23603 -4.29065 galactic Aql Second-epoch detections are separated by 0.6" and 2.0 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 J289.0990+02.7402 | 19:16:24.66 +02:44:47.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.890+/-0.036 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:24.58 +02:44:49.4: 12.52 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:24.58 +02:44:49.4: 12.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.0990+02.7402,2461186.7012,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.0990+02.7402 20260526.2012 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 05 26.2012 2461186.7012 11.44 19:16:39.50 +02:20:36.0
37.90548 -4.53196 galactic Aql Second-epoch detections are separated by 2.0" and 2.0 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 4267918867630266624 | 19:16:39.65 +02:20:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:39.50 +02:20:36.0: 12.53 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:39.50 +02:20:36.0: 12.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267918867630266624,2461186.7012,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267918867630266624 20260526.2012 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.45 19:13:50.94 +02:05:11.8
37.35287 -4.02722 galactic Aql Second-epoch detections are separated by 3.9" 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 J288.4573+02.0851 | 19:13:51.04 +02:05:09.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.313+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:50.94 +02:05:11.8: 12.51 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:50.94 +02:05:11.8: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.4573+02.0851,2461186.7012,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.4573+02.0851 20260526.2012 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.52 19:13:30.09 +02:25:17.7
37.61094 -3.79603 galactic Aql Second-epoch detections are separated by 1.4" and 2.1 pix
The object was found in VSX 3" ASASSN-V J191330.26+022518.4
Type: SR
# Max. Min./Amp. JD0 Period
13.300 g Y 0.340 g 2459512.52300 31.080000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:30.09 +02:25:17.7: 11.51 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:30.09 +02:25:17.7: 11.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191330.26+022518.4,2461186.7012,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191330.26+022518.4 20260526.2012 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.04 19:14:45.85 +02:21:28.7
37.69987 -4.10529 galactic Aql Second-epoch detections are separated by 2.6" and 2.3 pix
The object was found in VSX 8" Gaia DR3 4267948245208540928
Type: ROT
# Max. Min./Amp. JD0 Period
12.470 G 12.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:45.85 +02:21:28.7: 12.14 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:45.85 +02:21:28.7: 12.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267948245208540928,2461186.7012,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267948245208540928 20260526.2012 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.50 19:14:50.09 +02:31:41.3
37.85945 -4.04258 galactic Aql Second-epoch detections are separated by 5.1" 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 | Gaia DR3 4267963771464839552 | 19:14:50.10 +02:31:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:50.09 +02:31:41.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:50.09 +02:31:41.3: 12.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267963771464839552,2461186.7012,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267963771464839552 20260526.2012 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.26 19:14:38.84 +02:20:08.6
37.66660 -4.08963 galactic Aql Second-epoch detections are separated by 1.7" and 2.2 pix
The object was found in VSX 3" ASASSN-V J191438.92+022006.1
Type: SR
# Max. Min./Amp. JD0 Period
12.910 V 13.000 V 2457989.00000 354.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:38.84 +02:20:08.6: 12.52 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:38.84 +02:20:08.6: 12.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191438.92+022006.1,2461186.7012,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191438.92+022006.1 20260526.2012 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.49 19:12:51.82 +01:36:07.5
36.80804 -4.03126 galactic Aql Second-epoch detections are separated by 2.1" and 1.9 pix
The object was found in VSX23" ZTF J191251.17+013546.9
Type: EW
# Max. Min./Amp. JD0 Period
19.726 r Y 0.510 r 2458365.67120 0.495729200000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:51.82 +01:36:07.5: 12.48 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:51.82 +01:36:07.5: 12.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191251.17+013546.9,2461186.7012,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191251.17+013546.9 20260526.2012 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.19 19:11:31.35 +01:10:51.3
36.27875 -3.92673 galactic Aql Second-epoch detections are separated by 1.8" 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 | ATO J287.8811+01.1800 | 19:11:31.47 +01:10:48.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:31.35 +01:10:51.3: 12.49 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:31.35 +01:10:51.3: 12.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.8811+01.1800,2461186.7012,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.8811+01.1800 20260526.2012 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.69 19:14:41.34 +02:36:31.1
37.91425 -3.97317 galactic Aql Second-epoch detections are separated by 3.0" 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 | ATO J288.6787+02.6172 | 19:14:41.42 +02:36:28.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:41.34 +02:36:31.1: 12.77 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:41.34 +02:36:31.1: 12.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.6787+02.6172,2461186.7012,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6787+02.6172 20260526.2012 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 05 26.2012 2461186.7012 11.51 18:37:18.10 +08:22:25.0
38.81783 6.93132 galactic Oph Second-epoch detections are separated by 0.5" and 1.9 pix
The object was found in VSX 1" ASASSN-V J183718.15+082224.8
Type: SR
# Max. Min./Amp. JD0 Period
13.490 g Y 0.340 g 2458778.55000 525.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:37:18.10 +08:22:25.0: 12.51 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:37:18.10 +08:22:25.0: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J183718.15+082224.8,2461186.7012,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183718.15+082224.8 20260526.2012 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 05 26.2012 2461186.7012 11.38 19:19:41.66 +04:23:22.6
40.07650 -4.25694 galactic Aql Second-epoch detections are separated by 0.7" and 2.2 pix
The object was found in VSX 3" ASASSN-V J191941.88+042322.2
Type: SRS
# Max. Min./Amp. JD0 Period
13.460 V 13.630 V 2458185.11300 26.902000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:19:41.66 +04:23:22.6: 12.51 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:19:41.66 +04:23:22.6: 12.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191941.88+042322.2,2461186.7012,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191941.88+042322.2 20260526.2012 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 05 26.2012 2461186.7012 11.63 18:39:37.76 +09:03:36.6
39.69514 6.72296 galactic Oph Second-epoch detections are separated by 2.1" and 1.5 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 4479499019689913344 | 18:39:37.83 +09:03:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.722+/-0.032 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:39:37.76 +09:03:36.6: 12.49 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:39:37.76 +09:03:36.6: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4479499019689913344,2461186.7012,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4479499019689913344 20260526.2012 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.54 19:11:49.26 +01:00:08.6
36.15400 -4.07489 galactic Aql Second-epoch detections are separated by 2.7" and 2.2 pix
The object was found in VSX 5" ASASSN-V J191149.51+010005.2
Type: SR
# Max. Min./Amp. JD0 Period
14.160 V 14.750 V 2458431.38930 86.063949300000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:49.26 +01:00:08.6: 13.17 +/- 0.05 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:49.26 +01:00:08.6: 13.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191149.51+010005.2,2461186.7012,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191149.51+010005.2 20260526.2012 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 05 26.2012 2461186.7012 11.69 18:28:48.12 +07:21:45.0
36.95756 8.36441 galactic Oph Second-epoch detections are separated by 0.5" and 1.9 pix
The object was found in VSX 0" ASASSN-V J182848.10+072144.8
Type: L
# Max. Min./Amp. JD0 Period
12.940 V 13.260 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:28:48.12 +07:21:45.0: 12.75 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:28:48.12 +07:21:45.0: 12.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J182848.10+072144.8,2461186.7012,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182848.10+072144.8 20260526.2012 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 05 26.2012 2461186.7012 11.39 18:51:37.56 +05:21:58.2
37.73194 2.40235 galactic Ser Second-epoch detections are separated by 1.7" and 1.8 pix
The object was found in VSX 1" ASAS J185138+0521.9
Type: MISC
# Max. Min./Amp. JD0 Period
8.966 Ic Y 0.221 Ic 2452511.00000 84.660000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:51:37.56 +05:21:58.2: 12.46 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:51:37.56 +05:21:58.2: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.2012* 18 51 37.56 +05 21 58.2 11.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185138+0521.9,2461186.7012,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185138+0521.9 20260526.2012 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 05 26.2012 2461186.7012 11.35 18:49:58.07 +01:11:11.3
33.82038 0.86803 galactic Aql Second-epoch detections are separated by 0.9" and 1.9 pix
The object was found in VSX 1" NSVS J1849581+011113
Type: SR
# Max. Min./Amp. JD0 Period
15.065 g Y 0.467 g 2458319.75240 60.912002200000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:49:58.07 +01:11:11.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:49:58.07 +01:11:11.3: 12.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1849581+011113,2461186.7012,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1849581+011113 20260526.2012 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.38 19:22:08.49 +05:45:50.9
41.58073 -4.15632 galactic Aql Second-epoch detections are separated by 3.6" and 1.7 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 J290.5362+05.7645 | 19:22:08.70 +05:45:52.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:22:08.49 +05:45:50.9: 12.46 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:22:08.49 +05:45:50.9: 12.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J290.5362+05.7645,2461186.7012,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J290.5362+05.7645 20260526.2012 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 05 26.2012 2461186.7012 11.62 19:11:19.95 +01:47:21.7
36.79870 -3.60536 galactic Aql Second-epoch detections are separated by 5.0" and 1.5 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 J287.8334+01.7889 | 19:11:19.99 +01:47:19.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.351+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:19.95 +01:47:21.7: 12.75 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:19.95 +01:47:21.7: 12.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.8334+01.7889,2461186.7012,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.8334+01.7889 20260526.2012 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 05 26.2012 2461186.7012 11.05 19:16:29.23 +02:43:12.5
38.22104 -4.32024 galactic Aql Second-epoch detections are separated by 1.6" and 2.4 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 J289.1177+02.7105 | 19:16:29.40 +02:43:12.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:29.23 +02:43:12.5: 12.06 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:29.23 +02:43:12.5: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.1177+02.7105,2461186.7012,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.1177+02.7105 20260526.2012 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 05 26.2012 2461186.7012 11.03 19:22:12.56 +05:12:55.4
41.10191 -4.42729 galactic Aql Second-epoch detections are separated by 0.9" and 2.1 pix
The object was found in VSX 6" Gaia DR3 4292897950714683904
Type: L
# Max. Min./Amp. JD0 Period
18.120 G 18.400 G
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:22:12.56 +05:12:55.4: 12.08 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:22:12.56 +05:12:55.4: 12.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4292897950714683904,2461186.7012,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4292897950714683904 20260526.2012 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.04 19:13:12.33 +01:51:04.7
37.06929 -3.99263 galactic Aql Second-epoch detections are separated by 1.4" 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 | ATO J288.3022+01.8555 | 19:13:12.31 +01:51:07.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:12.33 +01:51:04.7: 12.06 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:12.33 +01:51:04.7: 12.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.3022+01.8555,2461186.7012,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.3022+01.8555 20260526.2012 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.40 19:16:19.17 +03:08:18.3
38.57372 -4.09004 galactic Aql Second-epoch detections are separated by 1.2" and 1.9 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 J289.0802+03.1273 | 19:16:19.30 +03:08:16.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.122+/-0.033 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:19.17 +03:08:18.3: 12.46 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:19.17 +03:08:18.3: 12.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.0802+03.1273,2461186.7012,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.0802+03.1273 20260526.2012 11.40CV 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 05 26.2012 2461186.7012 10.99 19:16:06.11 +03:01:38.7
38.44985 -4.09309 galactic Aql Second-epoch detections are separated by 0.9" and 1.9 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 J289.0197+03.0366 | 19:16:06.23 +03:01:38.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.153+/-0.048 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:16:06.11 +03:01:38.7: 12.06 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:16:06.11 +03:01:38.7: 12.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.0197+03.0366,2461186.7012,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.0197+03.0366 20260526.2012 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.85 18:50:50.13 +07:08:32.8
39.22763 3.38337 galactic Aql Second-epoch detections are separated by 3.7" and 2.4 pix
The object was found in VSX 0" ASASSN-V J185050.14+070832.5
Type: L
# Max. Min./Amp. JD0 Period
13.300 V 13.400 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:50:50.13 +07:08:32.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:50:50.13 +07:08:32.8: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185050.14+070832.5,2461186.7012,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185050.14+070832.5 20260526.2012 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 05 26.2012 2461186.7012 11.59 19:15:25.06 +02:55:03.2
38.27313 -3.99223 galactic Aql Second-epoch detections are separated by 1.8" and 2.2 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 J288.8553+02.9176 | 19:15:25.29 +02:55:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:25.06 +02:55:03.2: 12.76 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:25.06 +02:55:03.2: 12.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.8553+02.9176,2461186.7012,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.8553+02.9176 20260526.2012 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 05 26.2012 2461186.7012 11.10 19:21:45.86 +04:41:40.7
40.58791 -4.57186 galactic Aql Second-epoch detections are separated by 2.7" and 2.4 pix
The object was found in VSX20" ZTF J192146.14+044200.0
Type: EW
# Max. Min./Amp. JD0 Period
16.646 r Y 0.096 r 2458277.90830 0.761656600000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:21:45.86 +04:41:40.7: 12.06 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:21:45.86 +04:41:40.7: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192146.14+044200.0,2461186.7012,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192146.14+044200.0 20260526.2012 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.49 19:17:17.07 +04:08:08.3
39.57164 -3.84239 galactic Aql Second-epoch detections are separated by 4.3" 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 J289.3216+04.1352 | 19:17:17.19 +04:08:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.410+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:17.07 +04:08:08.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:17.07 +04:08:08.3: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.3216+04.1352,2461186.7012,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.3216+04.1352 20260526.2012 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.50 18:36:41.85 +09:56:19.7
40.16432 7.76121 galactic Oph Second-epoch detections are separated by 1.4" and 2.1 pix
The object was found in VSX 2" V0637 Oph
Type: LB:
# Max. Min./Amp. JD0 Period
13.600 pg 16.000 pg 730.000000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:36:41.85 +09:56:19.7: 12.45 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:36:41.85 +09:56:19.7: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0637 Oph,2461186.7012,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0637 Oph 20260526.2012 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.26 18:24:33.20 +07:37:50.4
36.72641 9.42684 galactic Oph Second-epoch detections are separated by 0.5" and 1.9 pix
The object was found in VSX 1" ASAS J182433+0737.8
Type: MISC
# Max. Min./Amp. JD0 Period
12.740 V Y 0.720 V 2452296.00000 67.499969000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:24:33.20 +07:37:50.4: 12.44 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:24:33.20 +07:37:50.4: 12.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J182433+0737.8,2461186.7012,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J182433+0737.8 20260526.2012 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.57 19:10:34.75 +01:41:13.0
36.62097 -3.48512 galactic Aql Second-epoch detections are separated by 1.5" and 1.9 pix
The object was found in VSX11" Gaia DR3 4267437556413621888
Type: E
# Max. Min./Amp. JD0 Period
19.080 G 19.580 G 0.397348000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:34.75 +01:41:13.0: 12.74 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:34.75 +01:41:13.0: 12.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267437556413621888,2461186.7012,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267437556413621888 20260526.2012 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 05 26.2012 2461186.7012 11.04 19:15:00.22 +02:24:14.4
37.76846 -4.13720 galactic Aql Second-epoch detections are separated by 3.4" and 1.9 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 J288.7419+02.4021 | 19:15:00.13 +02:24:12.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.729+/-0.046 (K)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:00.22 +02:24:14.4: 12.04 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:00.22 +02:24:14.4: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.7419+02.4021,2461186.7012,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.7419+02.4021 20260526.2012 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.42 19:11:22.02 +01:34:33.5
36.61270 -3.71097 galactic Aql Second-epoch detections are separated by 2.7" and 1.8 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 4267798363677840640 | 19:11:21.93 +01:34:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:22.02 +01:34:33.5: 12.46 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:22.02 +01:34:33.5: 12.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267798363677840640,2461186.7012,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267798363677840640 20260526.2012 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.11 19:11:11.94 +01:01:50.5
36.10777 -3.92374 galactic Aql Second-epoch detections are separated by 1.5" and 2.3 pix
The object was found in VSX 4" Gaia DR3 4267342173742211968
Type: L
# Max. Min./Amp. JD0 Period
15.680 G 15.930 G O
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:11.94 +01:01:50.5: 11.33 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:11.94 +01:01:50.5: 11.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267342173742211968,2461186.7012,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267342173742211968 20260526.2012 10.11CV 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 05 26.2012 2461186.7012 11.47 19:11:06.79 +00:53:52.5
35.97962 -3.96552 galactic Aql Second-epoch detections are separated by 4.3" and 2.4 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 J287.7809+00.9073 | 19:11:06.86 +00:53:49.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:11:06.79 +00:53:52.5: 12.45 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:11:06.79 +00:53:52.5: 12.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.7809+00.9073,2461186.7012,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.7809+00.9073 20260526.2012 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 05 26.2012 2461186.7012 11.12 19:13:39.05 +01:20:49.5
36.67150 -4.32312 galactic Aql Second-epoch detections are separated by 1.4" and 2.3 pix
The object was found in VSX 3" ZTF J191338.97+012047.2
Type: M
# Max. Min./Amp. JD0 Period
18.182 g Y 4.883 g 2457328.00000 268.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:39.05 +01:20:49.5: 12.44 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:39.05 +01:20:49.5: 12.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191338.97+012047.2,2461186.7012,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191338.97+012047.2 20260526.2012 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.35 19:14:46.24 +02:14:58.2
37.60408 -4.15668 galactic Aql Second-epoch detections are separated by 1.3" and 2.0 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 J288.6951+02.2520 | 19:14:46.29 +02:14:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:46.24 +02:14:58.2: 12.46 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:46.24 +02:14:58.2: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.6951+02.2520,2461186.7012,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6951+02.2520 20260526.2012 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.89 19:10:33.22 +01:14:59.6
36.22890 -3.67990 galactic Aql Second-epoch detections are separated by 0.8" and 2.0 pix
The object was found in VSX 3" ZTF J191033.35+011456.6
Type: SR
# Max. Min./Amp. JD0 Period
13.760 g Y 0.163 g 2458350.78020 30.301658800000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:33.22 +01:14:59.6: 12.03 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:33.22 +01:14:59.6: 12.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191033.35+011456.6,2461186.7012,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191033.35+011456.6 20260526.2012 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.53 19:13:04.23 +02:15:36.6
37.41767 -3.77470 galactic Aql Second-epoch detections are separated by 2.0" and 2.4 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 J288.2683+02.2599 | 19:13:04.39 +02:15:35.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:04.23 +02:15:36.6: 12.73 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:04.23 +02:15:36.6: 12.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.2683+02.2599,2461186.7012,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.2683+02.2599 20260526.2012 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.52 18:22:02.19 +08:40:14.8
37.39350 10.44567 galactic Oph Second-epoch detections are separated by 1.9" and 1.8 pix
The object was found in VSX 2" ASASSN-V J182202.04+084015.1
Type: SR
# Max. Min./Amp. JD0 Period
13.140 V 13.400 V 2457223.00000 743.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:22:02.19 +08:40:14.8: 12.81 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:22:02.19 +08:40:14.8: 12.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J182202.04+084015.1,2461186.7012,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182202.04+084015.1 20260526.2012 11.52CV 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 05 26.2012 2461186.7012 11.48 19:13:06.88 +01:32:11.9
36.77864 -4.11703 galactic Aql Second-epoch detections are separated by 0.5" and 2.0 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 J288.2874+01.5454 | 19:13:06.84 +01:32:11.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.882+/-0.035 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:06.88 +01:32:11.9: 12.44 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:06.88 +01:32:11.9: 12.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.2874+01.5454,2461186.7012,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.2874+01.5454 20260526.2012 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.19 19:12:49.69 +01:26:14.7
36.65731 -4.09899 galactic Aql Second-epoch detections are separated by 1.2" and 1.9 pix
The object was found in VSX 4" ASASSN-V J191249.89+012612.3
Type: SR
# Max. Min./Amp. JD0 Period
13.770 V 14.090 V 2458340.65020 32.196636200000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:49.69 +01:26:14.7: 12.74 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:49.69 +01:26:14.7: 12.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191249.89+012612.3,2461186.7012,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191249.89+012612.3 20260526.2012 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.10 19:10:23.88 +01:29:27.3
36.42565 -3.53481 galactic Aql Second-epoch detections are separated by 1.0" and 2.1 pix
The object was found in VSX 3" ZTF J191023.97+012924.6
Type: SR
# Max. Min./Amp. JD0 Period
13.547 g Y 0.189 g 2458377.98710 184.608897400000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:10:23.88 +01:29:27.3: 12.01 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:10:23.88 +01:29:27.3: 12.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191023.97+012924.6,2461186.7012,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191023.97+012924.6 20260526.2012 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.10 18:38:03.01 +09:23:34.2
39.82027 7.22004 galactic Oph Second-epoch detections are separated by 0.2" and 1.8 pix
The object was found in VSX 0" V0649 Oph
Type: LB
# Max. Min./Amp. JD0 Period
12.070 V Y 0.360 V 2452598.00000 138.888885000000 M6.5
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:38:03.01 +09:23:34.2: 11.28 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:38:03.01 +09:23:34.2: 10.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0649 Oph,2461186.7012,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0649 Oph 20260526.2012 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.12 19:13:27.19 +01:53:34.7
37.13490 -4.02844 galactic Aql Second-epoch detections are separated by 1.6" and 2.4 pix
The object was found in VSX 1" ASASSN-V J191327.20+015333.6
Type: SRS
# Max. Min./Amp. JD0 Period
13.110 V 13.210 V 2457820.13400 23.215000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:13:27.19 +01:53:34.7: 12.48 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:13:27.19 +01:53:34.7: 12.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191327.20+015333.6,2461186.7012,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191327.20+015333.6 20260526.2012 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.37 19:17:48.87 +03:00:04.3
38.62456 -4.48444 galactic Aql Second-epoch detections are separated by 2.0" and 2.0 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 J289.4500+03.0133 | 19:17:49.08 +03:00:05.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:17:48.87 +03:00:04.3: 12.44 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:17:48.87 +03:00:04.3: 12.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J289.4500+03.0133,2461186.7012,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.4500+03.0133 20260526.2012 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 10.14 19:12:37.66 +02:43:00.2
37.77286 -3.46645 galactic Aql Second-epoch detections are separated by 0.3" and 2.0 pix
The object was found in VSX 3" ASAS J191238+0243.0
Type: MISC
# Max. Min./Amp. JD0 Period
12.030 V Y 0.590 V 2452247.80000 58.065865000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:37.66 +02:43:00.2: 11.30 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:37.66 +02:43:00.2: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191238+0243.0,2461186.7012,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J191238+0243.0 20260526.2012 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.05 19:12:13.89 +02:11:25.3
37.25898 -3.62067 galactic Aql Second-epoch detections are separated by 1.5" and 2.0 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 J288.0472+02.1836 | 19:12:13.98 +02:11:24.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.351+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:13.89 +02:11:25.3: 11.98 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:13.89 +02:11:25.3: 12.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.0472+02.1836,2461186.7012,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.0472+02.1836 20260526.2012 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 05 26.2012 2461186.7012 11.37 19:15:02.53 +02:19:30.8
37.70279 -4.18202 galactic Aql Second-epoch detections are separated by 3.0" 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 | Gaia DR3 4267945015392869888 | 19:15:02.51 +02:19:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.934+/-0.038 (M)
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:02.53 +02:19:30.8: 12.42 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:02.53 +02:19:30.8: 12.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267945015392869888,2461186.7012,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267945015392869888 20260526.2012 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.23 19:15:50.62 +02:48:17.6
38.22210 -4.13858 galactic Aql Second-epoch detections are separated by 3.6" and 1.4 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 J288.9566+02.8084 | 19:15:50.77 +02:48:12.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:15:50.62 +02:48:17.6: 12.38 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:15:50.62 +02:48:17.6: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J288.9566+02.8084,2461186.7012,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.9566+02.8084 20260526.2012 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 05 26.2012 2461186.7012 10.87 19:12:48.99 +01:02:31.4
36.30375 -4.27783 galactic Aql Second-epoch detections are separated by 0.8" and 1.9 pix
The object was found in VSX 3" ASASSN-V J191249.17+010230.0
Type: L
# Max. Min./Amp. JD0 Period
12.870 V 13.320 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:48.99 +01:02:31.4: 12.02 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:48.99 +01:02:31.4: 12.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191249.17+010230.0,2461186.7012,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191249.17+010230.0 20260526.2012 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 05 26.2012 2461186.7012 11.32 18:23:41.32 +07:53:52.2
36.87285 9.73733 galactic Oph Second-epoch detections are separated by 3.2" and 1.8 pix
The object was found in VSX 3" ASASSN-V J182341.16+075350.6
Type: L:
# Max. Min./Amp. JD0 Period
12.560 V 12.950 V
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:23:41.32 +07:53:52.2: 12.29 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:23:41.32 +07:53:52.2: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J182341.16+075350.6,2461186.7012,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182341.16+075350.6 20260526.2012 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 05 26.2012 2461186.7012 10.89 19:18:43.58 +03:12:54.7
38.92049 -4.58731 galactic Aql Second-epoch detections are separated by 0.7" and 2.1 pix
The object was found in VSX 4" ZTF J191843.77+031252.7
Type: SR
# Max. Min./Amp. JD0 Period
13.952 g Y 0.174 g 2458654.64230 52.058464900000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:18:43.58 +03:12:54.7: 12.00 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:18:43.58 +03:12:54.7: 12.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191843.77+031252.7,2461186.7012,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191843.77+031252.7 20260526.2012 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.46 19:08:34.97 +00:58:07.9
35.75252 -3.37077 galactic Aql Second-epoch detections are separated by 3.1" and 2.6 pix
The object was found in VSX18" Gaia DR2 4267279359831357312
Type: M
# Max. Min./Amp. JD0 Period
17.054 r Y 2.965 r 2458377.20530 511.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:34.97 +00:58:07.9: 12.73 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:34.97 +00:58:07.9: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR2 4267279359831357312,2461186.7012,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR2 4267279359831357312 20260526.2012 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 05 26.2012 2461186.7012 11.80 18:39:04.66 +09:01:25.9
39.60124 6.82867 galactic Oph Second-epoch detections are separated by 1.6" and 2.0 pix
The object was found in VSX 1" ASASSN-V J183904.63+090125.0
Type: SR
# Max. Min./Amp. JD0 Period
12.850 V 12.950 V 2457901.00400 33.190000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:39:04.66 +09:01:25.9: 12.72 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:39:04.66 +09:01:25.9: 12.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J183904.63+090125.0,2461186.7012,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183904.63+090125.0 20260526.2012 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.03 19:18:33.71 +03:04:14.5
38.77290 -4.61775 galactic Aql Second-epoch detections are separated by 1.6" and 2.2 pix
The object was found in VSX 4" ASASSN-V J191833.91+030412.5
Type: SR
# Max. Min./Amp. JD0 Period
13.540 g Y 0.130 g 2458915.89500 326.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:18:33.71 +03:04:14.5: 11.98 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:18:33.71 +03:04:14.5: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J191833.91+030412.5,2461186.7012,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191833.91+030412.5 20260526.2012 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2012 2461186.7012 11.00 19:12:10.31 +01:05:15.9
36.27036 -4.11368 galactic Aql Second-epoch detections are separated by 3.3" and 2.0 pix
The object was found in VSX22" Gaia DR3 4267340593238376704
Type: E
# Max. Min./Amp. JD0 Period
17.520 G 17.800 G 0.588770000000 F
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:12:10.31 +01:05:15.9: 11.95 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:12:10.31 +01:05:15.9: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267340593238376704,2461186.7012,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267340593238376704 20260526.2012 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461125.98172973 26.03.2026 11:33:31.449 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
First image: 2461125.98172973 26.03.2026 11:33:31.449 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Last image: 2461186.70137510 26.05.2026 04:49:48.809 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
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: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13836
Objects passed selection criteria: 13769
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 9504.5
Average stars matched: 9305.75 (97.9089 %)
Memory usage VmPeak: 121280 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:52:28 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: 2461125.98172973 26.03.2026 11:33:31.449 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
First image: 2461125.98172973 26.03.2026 11:33:31.449 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Last image: 2461186.70137510 26.05.2026 04:49:48.809 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 308
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 24 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 115719
Objects passed selection criteria: 115372
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 77769.8
Average stars matched: 75238.2 (96.7449 %)
Memory usage VmPeak: 2025324 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:56:30 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.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/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.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: 2461186.70096229
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits exists and is non-empty
Saving wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits to local_wcs_cache/
'wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits' -> 'local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits'
wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits exists and is non-empty
Saving wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits to local_wcs_cache/
'wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits' -> 'local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits'
wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits'
wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits (1st reference image)
verification OK: wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:27.468 +05:59:57.13 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits (1st new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:24.533 +06:00:16.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:27.468 +05:59:57.13
Second-epoch image center 18:51:24.533 +06:00:16.80
Angular distance between the image centers 0.0133 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits (2nd new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:23.797 +06:00:15.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:27.468 +05:59:57.13
Second-epoch image center 18:51:23.797 +06:00:15.19
Angular distance between the image centers 0.0160 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 18:51:24.533 +06:00:16.80
Second-epoch second image center 18:51:23.797 +06:00:15.19
Angular distance between the image centers 0.00308 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits &> /tmp/tmp.yGq6ukHwkD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits &> /tmp/tmp.jS3y2265GE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits &> /tmp/tmp.VcYdq2rRDq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits &> /tmp/tmp.4rrNP3FTxV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.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_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits and wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat
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_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits and wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits and wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat
The reference image (wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits) and catalog (wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat) found
'wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat' -> 'wcsmag.cat'
Read 19833 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9583 to 290.8726 deg, Dec +0.6588 to +11.2779 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 274.9583 to 290.8726 deg, Dec 0.6588 to 11.2779 deg
Loaded 13534 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): 10293 out of 11133 total matches.
Matched with Tycho-2 11133 out of 19833 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.890600
a=0.000000 b=1.000000 c=22.890600
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 19833 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9583 to 290.8726 deg, Dec +0.6588 to +11.2779 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 274.9583 to 290.8726 deg, Dec 0.6588 to 11.2779 deg
Loaded 13534 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): 10293 out of 11133 total matches.
Matched with Tycho-2 11133 out of 19833 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits:
Forced-photometry filter: calibrated wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits -> calib.txt_param_ref_wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits (aperture=6.6)
Read 14620 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6671 to 291.1475 deg, Dec +0.1975 to +11.6850 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 274.6671 to 291.1475 deg, Dec 0.1975 to 11.6850 deg
Loaded 15071 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): 9505 out of 10048 total matches.
Matched with Tycho-2 10048 out of 14620 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits:
Forced-photometry filter: calibrated wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits -> calib.txt_param_ref_wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
2.4 pix Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
3.7 pix fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
3.7 pix fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
2.5 pix wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
2.4 pix wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
Limiting magnitude estimates:
14.9 mag. Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
14.5 mag. Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
11.5 mag. fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
11.6 mag. fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
All-image limiting magnitude estimate: 11.5 (SNR ) 9.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yGq6ukHwkD (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1868, passed=19833
Got 19833 stars (including 17955 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat
util/solve_plate_with_UCAC5 got 19833 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 19146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 19146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 19146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits N_match=939 sigma_overall_arcsec=0.596 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.742 sigma_q3_arcsec=0.600 sigma_q4_arcsec=0.630 n_q1=188 n_q2=269 n_q3=264 n_q4=218 worst_quadrant_to_overall_ratio=1.246
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits -region wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jS3y2265GE (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_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits' -> 'wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1253, passed=14620
Got 14620 stars (including 13359 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat
util/solve_plate_with_UCAC5 got 14620 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 14182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 14185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 14179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 937 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits N_match=937 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.428 n_q1=202 n_q2=223 n_q3=297 n_q4=215 worst_quadrant_to_overall_ratio=1.004
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits -region wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VcYdq2rRDq (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_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.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_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=67, passed=1888
Got 1888 stars (including 1821 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat
util/solve_plate_with_UCAC5 got 1888 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010472 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 1832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 1832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 1832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits N_match=941 sigma_overall_arcsec=0.412 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.573 sigma_q3_arcsec=0.367 sigma_q4_arcsec=0.401 n_q1=207 n_q2=190 n_q3=406 n_q4=138 worst_quadrant_to_overall_ratio=1.392
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits -region wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4rrNP3FTxV (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_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.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_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=73, passed=1925
Got 1925 stars (including 1852 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat
util/solve_plate_with_UCAC5 got 1925 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010472 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.5)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 1846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.5)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 1842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 1842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits N_match=938 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.469 sigma_q2_arcsec=0.799 sigma_q3_arcsec=0.337 sigma_q4_arcsec=0.389 n_q1=215 n_q2=185 n_q3=395 n_q4=143 worst_quadrant_to_overall_ratio=1.903
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits -region wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat.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=Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits sigma_overall=0.596 worst_q_ratio=1.246
ref2=Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits sigma_overall=0.434 worst_q_ratio=1.004
new1=fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits sigma_overall=0.412 worst_q_ratio=1.392
new2=fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits sigma_overall=0.420 worst_q_ratio=1.903
reference average sigma_overall=0.515 worst_q_ratio=1.125
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707_astrometric_residuals.png (939 matched stars from wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233_astrometric_residuals.png (937 matched stars from wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094_astrometric_residuals.png (941 matched stars from wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095_astrometric_residuals.png (938 matched stars from wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-13_20.00sec_-0.00C_LIGHTs_0094.fits'
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q1b1x1_235029_TTUQ1b1x1_2026427_acH3Q4rV/wcs_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095.fits'
Preparing the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ser-04-Q1b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:14:17.36 +00:42:39.5: 99.00 +/- 99.00 edge
Forced photometry on wcs_Ser-04-Q1b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:14:17.36 +00:42:39.5: 9.70 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 19:14:17.36 +00:42:39.5: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20792_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 20792_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 20793_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 20793_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:20:39.39 +02:47:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 00755_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 00755_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:11:56.58 +01:13:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20461_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 20461_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:21:44.26 +04:09:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07169_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 07169_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:19:14.29 +05:06:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17506_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 17506_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:47:13.66 +10:33:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17740_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 17740_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176403_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176403_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176406_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176406_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176407_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176407_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:10:52.21 +00:47:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 4.615 4267311284322656512 287.71837359237 +00.79052455419 10.9060 9.6945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176410_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176410_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 176412_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176412_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 176415_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176415_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:20:03.91 +02:19:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176417_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176417_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:21:28.02 +02:49:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176419_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176419_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 176420_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176420_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:20:29.05 +02:06:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176422_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176422_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:16:30.48 +01:23:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176424_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176424_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 176425_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176425_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:20:24.50 +01:16:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176426_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176426_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:19:59.33 +02:23:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176427_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176427_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:20:19.45 +02:25:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176428_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176428_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:17:22.93 +01:41:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176430_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176430_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176431_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176431_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176432_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176432_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:18:01.09 +01:43:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176433_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176433_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:28:51.14 +06:17:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176434_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176434_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:38:17.56 +08:13:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176436_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176436_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:21:11.98 +01:48:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176437_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176437_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 176440_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176440_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:16:22.56 +01:28:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176442_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176442_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 176444_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176444_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176448_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176448_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176449_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176449_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:43:46.89 +10:53:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176451_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176451_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:24:01.11 +07:23:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176454_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176454_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 176455_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176455_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 176456_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176456_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:25:31.03 +08:01:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 176457_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176457_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176458_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176458_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176460_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176460_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 176461_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176461_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 176462_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176462_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:35:40.87 +09:18:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176463_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176463_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:34:04.45 +08:52:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176464_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176464_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:36:31.23 +09:05:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 176465_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176465_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:40:27.86 +08:52:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176468_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176468_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 176469_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176469_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:09:29.40 +01:27:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176470_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176470_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 176476_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176476_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:55:30.14 +06:38:04.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 176478_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176478_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 176479_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176479_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 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 176480_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176480_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 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 176482_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 176482_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 170443_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 170443_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:30:12.49 +07:13:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12981_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 12981_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 46825_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 46825_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 26991_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 26991_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 01249_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 01249_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 167882_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 167882_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 02194_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02194_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 168085_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 168085_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 168247_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 168247_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 19168_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 19168_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 140308_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 140308_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 168669_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 168669_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 03805_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03805_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 23420_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 23420_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 04326_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04326_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 07547_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 07547_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 12964_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 12964_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 01505_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 01505_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02444_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02444_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 03498_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03498_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 04298_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04298_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 98214_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 98214_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 105598_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 105598_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 42467_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 42467_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 60330_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 60330_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 102094_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 102094_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:52:04.53 +08:15:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17863_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 17863_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 33461_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 33461_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:18:11.82 +03:42:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94070_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 94070_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 57068_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 57068_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 137791_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 137791_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 09445_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 09445_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:14:22.64 +01:46:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24622_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 24622_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 32234_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 32234_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 51413_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 51413_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:21:42.38 +04:56:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12112_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 12112_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:13:27.67 +02:03:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27793_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 27793_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 17605_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 17605_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 169242_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 169242_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 13998_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 13998_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 29034_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 29034_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 10325_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10325_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02039_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 02039_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:12:12.10 +00:58:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116643_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 116643_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:44:20.55 +10:33:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06016_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 06016_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02294_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 02294_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:12:06.19 +01:00:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04327_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04327_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 129722_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 129722_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 168969_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 168969_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 14067_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 14067_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 01936_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 01936_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:09:48.07 +00:59:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32937_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 32937_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 151712_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 151712_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 124239_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 124239_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:49:01.14 +09:54:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29968_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 29968_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 100371_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 100371_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 122251_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 122251_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02358_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02358_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 13697_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 13697_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 08314_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 08314_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 16678_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 16678_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 27158_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 27158_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:43:47.32 +03:23:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03991_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 03991_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:11:56.58 +01:13:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28725_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 28725_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 13357_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 13357_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 109681_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 109681_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 04693_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04693_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 15443_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15443_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 11755_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 11755_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 168140_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 168140_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 83037_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 83037_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:50:34.88 +07:07:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127739_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 127739_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:31:02.66 +09:40:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168097_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 168097_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 05504_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 05504_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 10467_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10467_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 09094_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 09094_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 15045_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15045_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 03302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 24351_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 24351_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 53917_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 53917_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:19:14.27 +05:06:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130086_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 130086_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 30813_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 30813_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:17:21.70 +03:30:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167745_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 167745_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 28609_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 28609_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 16760_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 16760_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:13:34.13 +02:30:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13648_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 13648_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02249_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02249_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 15486_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15486_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 03303_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03303_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 167415_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 167415_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:29:55.83 +09:50:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31471_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 31471_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 31508_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 31508_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02978_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02978_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 167101_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 167101_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 38300_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 38300_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 102960_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 102960_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:28:58.91 +08:19:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21805_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 21805_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 46489_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 46489_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:52:35.02 +04:41:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15332_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15332_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 17468_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 17468_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 10922_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10922_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 25735_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 25735_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 143221_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 143221_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 109998_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 109998_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 102277_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 102277_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 131457_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 131457_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 10058_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10058_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 62517_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 62517_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 05543_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 05543_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 28948_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 28948_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 22797_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 22797_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02082_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 02082_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 126895_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 126895_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 03039_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03039_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 98725_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 98725_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 54937_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 54937_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:21:04.95 +05:22:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53813_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 53813_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 14995_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 14995_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 13743_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 13743_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 08368_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 08368_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 22288_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 22288_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 04183_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04183_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 08968_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 08968_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 12226_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 12226_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 33155_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 33155_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 29998_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 29998_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 43774_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 43774_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 33556_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 33556_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 01480_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 01480_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 19986_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 19986_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 20234_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 20234_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 105189_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 105189_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:01:23.38 +08:19:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03797_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03797_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 135402_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 135402_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 138685_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 138685_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 07204_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 07204_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 03332_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03332_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 24279_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 24279_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 27302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 27302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 27796_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 27796_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 10962_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10962_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 08633_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 08633_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 01686_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 01686_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 17843_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 17843_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:14:36.96 +02:33:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04987_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04987_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 19588_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 19588_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 33435_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 33435_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 05415_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 05415_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 111685_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 111685_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 21192_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 21192_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 22124_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 22124_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 91699_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 91699_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 14383_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 14383_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 20274_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 20274_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 15563_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15563_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 12715_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 12715_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 96693_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 96693_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:36:05.04 +07:57:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16004_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 16004_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 15502_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15502_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 17608_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 17608_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 39811_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 39811_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:18:12.45 +04:07:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151085_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 151085_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:42:49.70 +10:44:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15401_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15401_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 07745_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 07745_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 03829_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 03829_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 18541_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 18541_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 26571_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 26571_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:15:30.84 +03:18:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06494_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 06494_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:12:17.26 +01:29:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103955_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 103955_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 43419_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 43419_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 137227_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 137227_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02429_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02429_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 86516_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 86516_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 55754_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 55754_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 02633_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02633_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 63302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 63302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 09532_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 09532_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 19758_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 19758_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 55053_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 55053_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 10055_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10055_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 106378_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 106378_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:47:13.66 +10:33:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25320_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 25320_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 23992_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 23992_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 83197_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 83197_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 117279_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 117279_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:37:19.37 +10:25:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22247_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 22247_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 47594_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 47594_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 39791_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 39791_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 123992_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 123992_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 91338_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 91338_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 56569_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 56569_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
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Considering the candidate 08380_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 08380_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 15929_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15929_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 32331_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 32331_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:19:08.28 +03:37:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07494_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 07494_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 00302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 00302_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 01633_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 01633_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 05248_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 05248_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 14437_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 14437_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 04297_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 04297_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
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Considering the candidate 14518_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 14518_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111289_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 111289_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07150_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 07150_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06155_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 06155_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06596_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 06596_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132248_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 132248_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30568_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 30568_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10662_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 10662_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23705_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 23705_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19304_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 19304_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13586_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 13586_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15247_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 15247_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20943_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 20943_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02658_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02658_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95990_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 95990_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26525_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 26525_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02081_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02081_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137340_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 137340_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24620_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 24620_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02955_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
Preparing report for the candidate 02955_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38097_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 38097_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:56:13.83 +04:12:11.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13784_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 13784_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 19:13:42.68 +02:17:35.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25264_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095
The candidate 25264_fd_Ser-04-Q1b1x1_2026-05-25_23-49-48_20.00sec_-0.00C_LIGHTs_0095 did not pass the final checks
**** FOUND 18:20:52.22 +03:22:37.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 254s
Prepared the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:11:11.94 +01:01:50.5
19:10:18.03 +00:51:17.2
19:10:34.26 +00:53:03.3
19:11:13.06 +00:53:34.5
19:11:06.79 +00:53:52.5
19:08:55.77 +00:54:57.0
19:08:34.97 +00:58:07.9
19:08:31.32 +00:59:05.4
19:12:38.61 +00:58:49.9
19:09:25.59 +01:00:44.5
19:11:49.26 +01:00:08.6
19:12:22.67 +01:00:55.9
18:49:58.07 +01:11:11.3
19:12:48.99 +01:02:31.4
19:12:10.31 +01:05:15.9
19:09:15.41 +01:05:04.1
19:11:33.77 +01:05:12.0
19:12:22.99 +01:07:09.0
19:12:04.74 +01:07:02.9
19:09:52.82 +01:08:27.6
19:11:44.59 +01:09:26.4
19:09:22.42 +01:12:15.4
19:09:40.50 +01:11:06.0
19:11:31.35 +01:10:51.3
19:12:24.66 +01:12:47.1
19:10:33.22 +01:14:59.6
19:10:45.87 +01:14:45.1
19:12:03.17 +01:14:11.7
19:11:37.11 +01:14:14.0
19:10:43.80 +01:16:32.7
19:08:54.40 +01:19:41.5
19:13:39.05 +01:20:49.5
19:09:49.48 +01:25:27.0
19:08:42.78 +01:22:46.1
19:12:47.48 +01:23:15.5
19:13:43.37 +01:24:35.7
19:12:49.69 +01:26:14.7
19:10:23.88 +01:29:27.3
19:13:06.88 +01:32:11.9
19:12:45.60 +01:33:22.1
19:11:22.02 +01:34:33.5
19:12:06.38 +01:35:19.2
19:12:51.82 +01:36:07.5
19:12:33.70 +01:40:10.4
19:09:58.61 +01:40:52.7
19:10:34.75 +01:41:13.0
19:15:51.47 +01:41:49.2
19:11:25.00 +01:44:06.8
19:12:48.43 +01:45:53.5
19:11:19.95 +01:47:21.7
18:34:56.38 +08:10:00.6
19:13:12.33 +01:51:04.7
19:14:06.44 +01:50:04.1
19:12:58.76 +01:51:37.3
18:37:18.10 +08:22:25.0
19:13:23.64 +01:52:46.4
19:13:27.19 +01:53:34.7
19:12:20.36 +01:55:15.4
19:11:04.68 +01:56:12.2
18:34:15.36 +09:04:11.0
18:36:44.34 +09:00:04.4
18:22:02.19 +08:40:14.8
18:22:48.75 +08:35:49.3
19:13:42.31 +01:59:41.7
18:30:20.44 +09:58:11.0
19:14:28.31 +02:02:54.2
18:36:41.85 +09:56:19.7
19:13:50.94 +02:05:11.8
19:15:06.08 +02:06:40.6
18:37:51.03 +09:35:49.2
19:13:51.54 +02:07:15.2
18:35:59.12 +09:27:39.2
18:38:03.01 +09:23:34.2
19:15:31.50 +02:08:35.3
18:37:18.07 +09:11:21.6
19:12:13.89 +02:11:25.3
19:15:17.09 +02:11:14.3
19:14:13.57 +02:11:10.8
18:39:37.76 +09:03:36.6
18:39:04.66 +09:01:25.9
19:15:59.79 +02:11:07.1
18:35:40.81 +08:58:00.1
18:38:25.02 +08:58:31.5
19:15:41.66 +02:12:58.8
18:39:14.92 +08:50:13.6
19:12:54.83 +02:13:22.8
19:12:41.25 +02:15:06.7
19:14:46.24 +02:14:58.2
19:13:04.23 +02:15:36.6
19:15:29.29 +02:19:06.1
19:16:17.63 +02:19:17.0
18:49:58.85 +10:41:08.6
19:15:02.53 +02:19:30.8
19:15:07.67 +02:21:22.9
19:14:38.84 +02:20:08.6
19:12:05.39 +02:21:10.6
19:13:49.37 +02:21:19.6
19:14:45.85 +02:21:28.7
19:16:39.50 +02:20:36.0
19:15:00.22 +02:24:14.4
19:13:30.09 +02:25:17.7
19:15:33.78 +02:27:12.9
19:15:20.01 +02:31:03.6
19:12:18.71 +02:33:26.4
19:14:50.09 +02:31:41.3
19:16:44.49 +02:32:42.0
19:14:41.34 +02:36:31.1
19:16:36.52 +02:39:51.6
19:12:37.66 +02:43:00.2
19:16:09.46 +02:41:47.4
19:16:29.23 +02:43:12.5
19:15:35.37 +02:44:04.2
19:15:54.53 +02:44:55.9
19:16:24.58 +02:44:49.4
19:15:50.62 +02:48:17.6
19:15:35.44 +02:49:51.5
19:14:42.73 +02:51:60.0
19:17:08.71 +02:53:14.9
19:15:25.06 +02:55:03.2
19:16:43.76 +02:53:56.7
19:16:28.64 +02:56:23.9
19:15:23.96 +03:00:51.4
19:17:48.87 +03:00:04.3
19:16:06.11 +03:01:38.7
19:17:00.90 +03:03:21.5
19:15:05.00 +03:03:55.6
19:18:33.71 +03:04:14.5
19:17:25.72 +03:04:12.4
19:16:19.17 +03:08:18.3
19:14:21.38 +03:10:09.9
19:18:43.58 +03:12:54.7
19:16:08.18 +03:15:01.8
19:17:03.27 +03:16:34.1
19:17:26.16 +03:19:46.5
19:17:17.99 +03:18:40.6
19:19:09.96 +03:21:17.4
19:19:09.82 +03:22:01.2
19:16:31.51 +03:23:26.8
19:16:18.18 +03:24:06.6
19:16:34.08 +03:27:26.8
19:15:59.29 +03:28:20.5
19:18:32.77 +03:33:36.4
19:19:05.82 +03:33:07.7
19:19:24.42 +03:36:24.1
19:16:59.69 +03:40:16.1
19:17:59.56 +03:41:43.2
19:15:59.03 +03:42:28.9
19:19:11.82 +03:42:32.2
19:20:58.87 +03:59:47.1
19:17:17.07 +04:08:08.3
19:18:53.87 +04:17:35.9
19:19:41.66 +04:23:22.6
19:20:54.22 +04:24:59.7
19:20:37.79 +04:38:35.2
19:21:45.86 +04:41:40.7
19:21:48.79 +05:07:49.7
19:22:12.56 +05:12:55.4
18:51:37.56 +05:21:58.2
19:21:37.63 +05:20:33.3
19:21:45.03 +05:34:08.4
19:22:17.57 +05:43:17.0
19:22:08.49 +05:45:50.9
18:50:50.13 +07:08:32.8
18:28:48.12 +07:21:45.0
18:24:33.20 +07:37:50.4
18:29:40.19 +07:38:22.2
18:37:19.86 +07:47:43.9
18:23:41.32 +07:53:52.2
18:30:48.38 +08:01:23.0
18:36:18.15 +08:04:10.9
########### Completed Ser-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:13:51.54 +02:07:15.2
19:20:37.79 +04:38:35.2
19:16:08.18 +03:15:01.8
19:10:18.03 +00:51:17.2
19:08:31.32 +00:59:05.4
19:16:36.52 +02:39:51.6
18:39:14.92 +08:50:13.6
19:09:40.50 +01:11:06.0
19:15:23.96 +03:00:51.4
19:12:03.17 +01:14:11.7
19:12:06.38 +01:35:19.2
19:15:06.08 +02:06:40.6
19:11:13.06 +00:53:34.5
19:12:22.67 +01:00:55.9
19:11:44.59 +01:09:26.4
19:10:45.87 +01:14:45.1
18:30:48.38 +08:01:23.0
19:18:53.87 +04:17:35.9
19:21:45.03 +05:34:08.4
19:16:44.49 +02:32:42.0
18:37:19.86 +07:47:43.9
19:21:37.63 +05:20:33.3
18:35:40.81 +08:58:00.1
19:17:25.72 +03:04:12.4
19:19:24.42 +03:36:24.1
19:17:26.16 +03:19:46.5
19:12:18.71 +02:33:26.4
19:15:41.66 +02:12:58.8
19:16:18.18 +03:24:06.6
19:12:58.76 +01:51:37.3
19:13:43.37 +01:24:35.7
19:11:37.11 +01:14:14.0
18:37:51.03 +09:35:49.2
19:12:54.83 +02:13:22.8
19:16:59.69 +03:40:16.1
18:49:58.85 +10:41:08.6
19:16:34.08 +03:27:26.8
18:34:56.38 +08:10:00.6
18:30:20.44 +09:58:11.0
19:09:25.59 +01:00:44.5
19:14:13.57 +02:11:10.8
19:12:33.70 +01:40:10.4
19:15:33.78 +02:27:12.9
19:19:09.82 +03:22:01.2
19:15:31.50 +02:08:35.3
18:34:15.36 +09:04:11.0
19:10:43.80 +01:16:32.7
19:12:05.39 +02:21:10.6
19:13:42.31 +01:59:41.7
19:08:42.78 +01:22:46.1
19:13:23.64 +01:52:46.4
19:12:48.43 +01:45:53.5
19:16:17.63 +02:19:17.0
19:12:22.99 +01:07:09.0
19:15:05.00 +03:03:55.6
19:19:09.96 +03:21:17.4
19:15:17.09 +02:11:14.3
19:12:38.61 +00:58:49.9
19:13:49.37 +02:21:19.6
19:12:04.74 +01:07:02.9
19:18:32.77 +03:33:36.4
19:19:05.82 +03:33:07.7
19:09:15.41 +01:05:04.1
19:20:58.87 +03:59:47.1
19:14:42.73 +02:51:60.0
19:15:07.67 +02:21:22.9
19:15:20.01 +02:31:03.6
19:12:20.36 +01:55:15.4
19:14:21.38 +03:10:09.9
18:36:44.34 +09:00:04.4
18:35:59.12 +09:27:39.2
19:14:06.44 +01:50:04.1
19:22:17.57 +05:43:17.0
19:12:47.48 +01:23:15.5
19:16:31.51 +03:23:26.8
19:16:28.64 +02:56:23.9
19:11:33.77 +01:05:12.0
18:36:18.15 +08:04:10.9
19:21:48.79 +05:07:49.7
19:15:29.29 +02:19:06.1
19:15:59.79 +02:11:07.1
19:09:58.61 +01:40:52.7
19:16:43.76 +02:53:56.7
19:12:24.66 +01:12:47.1
19:11:25.00 +01:44:06.8
19:14:28.31 +02:02:54.2
19:17:59.56 +03:41:43.2
19:15:59.29 +03:28:20.5
19:20:54.22 +04:24:59.7
19:19:11.82 +03:42:32.2
19:10:34.26 +00:53:03.3
19:15:35.37 +02:44:04.2
19:15:54.53 +02:44:55.9
19:09:22.42 +01:12:15.4
18:37:18.07 +09:11:21.6
18:38:25.02 +08:58:31.5
19:12:45.60 +01:33:22.1
19:09:52.82 +01:08:27.6
19:17:00.90 +03:03:21.5
19:17:03.27 +03:16:34.1
19:17:17.99 +03:18:40.6
19:11:04.68 +01:56:12.2
19:15:51.47 +01:41:49.2
19:08:55.77 +00:54:57.0
19:08:54.40 +01:19:41.5
19:16:09.46 +02:41:47.4
19:15:59.03 +03:42:28.9
19:09:49.48 +01:25:27.0
18:22:48.75 +08:35:49.3
19:15:35.44 +02:49:51.5
19:17:08.71 +02:53:14.9
18:29:40.19 +07:38:22.2
19:12:41.25 +02:15:06.7
19:16:24.58 +02:44:49.4
19:16:39.50 +02:20:36.0
19:13:50.94 +02:05:11.8
19:13:30.09 +02:25:17.7
19:14:45.85 +02:21:28.7
19:14:50.09 +02:31:41.3
19:14:38.84 +02:20:08.6
19:12:51.82 +01:36:07.5
19:11:31.35 +01:10:51.3
19:14:41.34 +02:36:31.1
18:37:18.10 +08:22:25.0
19:19:41.66 +04:23:22.6
18:39:37.76 +09:03:36.6
19:11:49.26 +01:00:08.6
18:28:48.12 +07:21:45.0
18:51:37.56 +05:21:58.2
18:49:58.07 +01:11:11.3
19:22:08.49 +05:45:50.9
19:11:19.95 +01:47:21.7
19:16:29.23 +02:43:12.5
19:22:12.56 +05:12:55.4
19:13:12.33 +01:51:04.7
19:16:19.17 +03:08:18.3
19:16:06.11 +03:01:38.7
18:50:50.13 +07:08:32.8
19:15:25.06 +02:55:03.2
19:21:45.86 +04:41:40.7
19:17:17.07 +04:08:08.3
18:36:41.85 +09:56:19.7
18:24:33.20 +07:37:50.4
19:10:34.75 +01:41:13.0
19:15:00.22 +02:24:14.4
19:11:22.02 +01:34:33.5
19:11:11.94 +01:01:50.5
19:11:06.79 +00:53:52.5
19:13:39.05 +01:20:49.5
19:14:46.24 +02:14:58.2
19:10:33.22 +01:14:59.6
19:13:04.23 +02:15:36.6
18:22:02.19 +08:40:14.8
19:13:06.88 +01:32:11.9
19:12:49.69 +01:26:14.7
19:10:23.88 +01:29:27.3
18:38:03.01 +09:23:34.2
19:13:27.19 +01:53:34.7
19:17:48.87 +03:00:04.3
19:12:37.66 +02:43:00.2
19:12:13.89 +02:11:25.3
19:15:02.53 +02:19:30.8
19:15:50.62 +02:48:17.6
19:12:48.99 +01:02:31.4
18:23:41.32 +07:53:52.2
19:18:43.58 +03:12:54.7
19:08:34.97 +00:58:07.9
18:39:04.66 +09:01:25.9
19:18:33.71 +03:04:14.5
19:12:10.31 +01:05:15.9
###################################################################################
19:13:51.54 +02:07:15.2 -- not an asteroid (will add it to exclusion list)
19:20:37.79 +04:38:35.2 -- not an asteroid (will add it to exclusion list)
19:16:08.18 +03:15:01.8 -- not an asteroid (will add it to exclusion list)
19:10:18.03 +00:51:17.2 -- not an asteroid (will add it to exclusion list)
19:08:31.32 +00:59:05.4 -- not an asteroid (will add it to exclusion list)
19:16:36.52 +02:39:51.6 -- not an asteroid (will add it to exclusion list)
18:39:14.92 +08:50:13.6 -- not an asteroid (will add it to exclusion list)
19:09:40.50 +01:11:06.0 -- not an asteroid (will add it to exclusion list)
19:15:23.96 +03:00:51.4 -- not an asteroid (will add it to exclusion list)
19:12:03.17 +01:14:11.7 -- not an asteroid (will add it to exclusion list)
19:12:06.38 +01:35:19.2 -- not an asteroid (will add it to exclusion list)
19:15:06.08 +02:06:40.6 -- not an asteroid (will add it to exclusion list)
19:11:13.06 +00:53:34.5 -- not an asteroid (will add it to exclusion list)
19:12:22.67 +01:00:55.9 -- not an asteroid (will add it to exclusion list)
19:11:44.59 +01:09:26.4 -- not an asteroid (will add it to exclusion list)
19:10:45.87 +01:14:45.1 -- not an asteroid (will add it to exclusion list)
18:30:48.38 +08:01:23.0 -- not an asteroid (will add it to exclusion list)
19:18:53.87 +04:17:35.9 -- not an asteroid (will add it to exclusion list)
19:21:45.03 +05:34:08.4 -- not an asteroid (will add it to exclusion list)
19:16:44.49 +02:32:42.0 -- not an asteroid (will add it to exclusion list)
18:37:19.86 +07:47:43.9 -- not an asteroid (will add it to exclusion list)
19:21:37.63 +05:20:33.3 -- not an asteroid (will add it to exclusion list)
18:35:40.81 +08:58:00.1 -- not an asteroid (will add it to exclusion list)
19:17:25.72 +03:04:12.4 -- not an asteroid (will add it to exclusion list)
19:19:24.42 +03:36:24.1 -- not an asteroid (will add it to exclusion list)
19:17:26.16 +03:19:46.5 -- not an asteroid (will add it to exclusion list)
19:12:18.71 +02:33:26.4 -- not an asteroid (will add it to exclusion list)
19:15:41.66 +02:12:58.8 -- not an asteroid (will add it to exclusion list)
19:16:18.18 +03:24:06.6 -- not an asteroid (will add it to exclusion list)
19:12:58.76 +01:51:37.3 -- not an asteroid (will add it to exclusion list)
19:13:43.37 +01:24:35.7 -- not an asteroid (will add it to exclusion list)
19:11:37.11 +01:14:14.0 -- not an asteroid (will add it to exclusion list)
18:37:51.03 +09:35:49.2 -- not an asteroid (will add it to exclusion list)
19:12:54.83 +02:13:22.8 -- not an asteroid (will add it to exclusion list)
19:16:59.69 +03:40:16.1 -- not an asteroid (will add it to exclusion list)
18:49:58.85 +10:41:08.6 -- not an asteroid (will add it to exclusion list)
19:16:34.08 +03:27:26.8 -- not an asteroid (will add it to exclusion list)
18:34:56.38 +08:10:00.6 -- not an asteroid (will add it to exclusion list)
18:30:20.44 +09:58:11.0 -- not an asteroid (will add it to exclusion list)
19:09:25.59 +01:00:44.5 -- not an asteroid (will add it to exclusion list)
19:14:13.57 +02:11:10.8 -- not an asteroid (will add it to exclusion list)
19:12:33.70 +01:40:10.4 -- not an asteroid (will add it to exclusion list)
19:15:33.78 +02:27:12.9 -- not an asteroid (will add it to exclusion list)
19:19:09.82 +03:22:01.2 -- not an asteroid (will add it to exclusion list)
19:15:31.50 +02:08:35.3 -- not an asteroid (will add it to exclusion list)
18:34:15.36 +09:04:11.0 -- not an asteroid (will add it to exclusion list)
19:10:43.80 +01:16:32.7 -- not an asteroid (will add it to exclusion list)
19:12:05.39 +02:21:10.6 -- not an asteroid (will add it to exclusion list)
19:13:42.31 +01:59:41.7 -- not an asteroid (will add it to exclusion list)
19:08:42.78 +01:22:46.1 -- not an asteroid (will add it to exclusion list)
19:13:23.64 +01:52:46.4 -- not an asteroid (will add it to exclusion list)
19:12:48.43 +01:45:53.5 -- not an asteroid (will add it to exclusion list)
19:16:17.63 +02:19:17.0 -- not an asteroid (will add it to exclusion list)
19:12:22.99 +01:07:09.0 -- not an asteroid (will add it to exclusion list)
19:15:05.00 +03:03:55.6 -- not an asteroid (will add it to exclusion list)
19:19:09.96 +03:21:17.4 -- not an asteroid (will add it to exclusion list)
19:15:17.09 +02:11:14.3 -- not an asteroid (will add it to exclusion list)
19:12:38.61 +00:58:49.9 -- not an asteroid (will add it to exclusion list)
19:13:49.37 +02:21:19.6 -- not an asteroid (will add it to exclusion list)
19:12:04.74 +01:07:02.9 -- not an asteroid (will add it to exclusion list)
19:18:32.77 +03:33:36.4 -- not an asteroid (will add it to exclusion list)
19:19:05.82 +03:33:07.7 -- not an asteroid (will add it to exclusion list)
19:09:15.41 +01:05:04.1 -- not an asteroid (will add it to exclusion list)
19:20:58.87 +03:59:47.1 -- not an asteroid (will add it to exclusion list)
19:14:42.73 +02:51:60.0 -- not an asteroid (will add it to exclusion list)
19:15:07.67 +02:21:22.9 -- not an asteroid (will add it to exclusion list)
19:15:20.01 +02:31:03.6 -- not an asteroid (will add it to exclusion list)
19:12:20.36 +01:55:15.4 -- not an asteroid (will add it to exclusion list)
19:14:21.38 +03:10:09.9 -- not an asteroid (will add it to exclusion list)
18:36:44.34 +09:00:04.4 -- not an asteroid (will add it to exclusion list)
18:35:59.12 +09:27:39.2 -- not an asteroid (will add it to exclusion list)
19:14:06.44 +01:50:04.1 -- not an asteroid (will add it to exclusion list)
19:22:17.57 +05:43:17.0 -- not an asteroid (will add it to exclusion list)
19:12:47.48 +01:23:15.5 -- not an asteroid (will add it to exclusion list)
19:16:31.51 +03:23:26.8 -- not an asteroid (will add it to exclusion list)
19:16:28.64 +02:56:23.9 -- not an asteroid (will add it to exclusion list)
19:11:33.77 +01:05:12.0 -- not an asteroid (will add it to exclusion list)
18:36:18.15 +08:04:10.9 -- not an asteroid (will add it to exclusion list)
19:21:48.79 +05:07:49.7 -- not an asteroid (will add it to exclusion list)
19:15:29.29 +02:19:06.1 -- not an asteroid (will add it to exclusion list)
19:15:59.79 +02:11:07.1 -- not an asteroid (will add it to exclusion list)
19:09:58.61 +01:40:52.7 -- not an asteroid (will add it to exclusion list)
19:16:43.76 +02:53:56.7 -- not an asteroid (will add it to exclusion list)
19:12:24.66 +01:12:47.1 -- not an asteroid (will add it to exclusion list)
19:11:25.00 +01:44:06.8 -- not an asteroid (will add it to exclusion list)
19:14:28.31 +02:02:54.2 -- not an asteroid (will add it to exclusion list)
19:17:59.56 +03:41:43.2 -- not an asteroid (will add it to exclusion list)
19:15:59.29 +03:28:20.5 -- not an asteroid (will add it to exclusion list)
19:20:54.22 +04:24:59.7 -- not an asteroid (will add it to exclusion list)
19:19:11.82 +03:42:32.2 -- not an asteroid (will add it to exclusion list)
19:10:34.26 +00:53:03.3 -- not an asteroid (will add it to exclusion list)
19:15:35.37 +02:44:04.2 -- not an asteroid (will add it to exclusion list)
19:15:54.53 +02:44:55.9 -- not an asteroid (will add it to exclusion list)
19:09:22.42 +01:12:15.4 -- not an asteroid (will add it to exclusion list)
18:37:18.07 +09:11:21.6 -- not an asteroid (will add it to exclusion list)
18:38:25.02 +08:58:31.5 -- not an asteroid (will add it to exclusion list)
19:12:45.60 +01:33:22.1 -- not an asteroid (will add it to exclusion list)
19:09:52.82 +01:08:27.6 -- not an asteroid (will add it to exclusion list)
19:17:00.90 +03:03:21.5 -- not an asteroid (will add it to exclusion list)
19:17:03.27 +03:16:34.1 -- not an asteroid (will add it to exclusion list)
19:17:17.99 +03:18:40.6 -- not an asteroid (will add it to exclusion list)
19:11:04.68 +01:56:12.2 -- not an asteroid (will add it to exclusion list)
19:15:51.47 +01:41:49.2 -- not an asteroid (will add it to exclusion list)
19:08:55.77 +00:54:57.0 -- not an asteroid (will add it to exclusion list)
19:08:54.40 +01:19:41.5 -- not an asteroid (will add it to exclusion list)
19:16:09.46 +02:41:47.4 -- not an asteroid (will add it to exclusion list)
19:15:59.03 +03:42:28.9 -- not an asteroid (will add it to exclusion list)
19:09:49.48 +01:25:27.0 -- not an asteroid (will add it to exclusion list)
18:22:48.75 +08:35:49.3 -- not an asteroid (will add it to exclusion list)
19:15:35.44 +02:49:51.5 -- not an asteroid (will add it to exclusion list)
19:17:08.71 +02:53:14.9 -- not an asteroid (will add it to exclusion list)
18:29:40.19 +07:38:22.2 -- not an asteroid (will add it to exclusion list)
19:12:41.25 +02:15:06.7 -- not an asteroid (will add it to exclusion list)
19:16:24.58 +02:44:49.4 -- not an asteroid (will add it to exclusion list)
19:16:39.50 +02:20:36.0 -- not an asteroid (will add it to exclusion list)
19:13:50.94 +02:05:11.8 -- not an asteroid (will add it to exclusion list)
19:13:30.09 +02:25:17.7 -- not an asteroid (will add it to exclusion list)
19:14:45.85 +02:21:28.7 -- not an asteroid (will add it to exclusion list)
19:14:50.09 +02:31:41.3 -- not an asteroid (will add it to exclusion list)
19:14:38.84 +02:20:08.6 -- not an asteroid (will add it to exclusion list)
19:12:51.82 +01:36:07.5 -- not an asteroid (will add it to exclusion list)
19:11:31.35 +01:10:51.3 -- not an asteroid (will add it to exclusion list)
19:14:41.34 +02:36:31.1 -- not an asteroid (will add it to exclusion list)
18:37:18.10 +08:22:25.0 -- not an asteroid (will add it to exclusion list)
19:19:41.66 +04:23:22.6 -- not an asteroid (will add it to exclusion list)
18:39:37.76 +09:03:36.6 -- not an asteroid (will add it to exclusion list)
19:11:49.26 +01:00:08.6 -- not an asteroid (will add it to exclusion list)
18:28:48.12 +07:21:45.0 -- not an asteroid (will add it to exclusion list)
18:51:37.56 +05:21:58.2 -- not an asteroid (will add it to exclusion list)
18:49:58.07 +01:11:11.3 -- not an asteroid (will add it to exclusion list)
19:22:08.49 +05:45:50.9 -- not an asteroid (will add it to exclusion list)
19:11:19.95 +01:47:21.7 -- not an asteroid (will add it to exclusion list)
19:16:29.23 +02:43:12.5 -- not an asteroid (will add it to exclusion list)
19:22:12.56 +05:12:55.4 -- not an asteroid (will add it to exclusion list)
19:13:12.33 +01:51:04.7 -- not an asteroid (will add it to exclusion list)
19:16:19.17 +03:08:18.3 -- not an asteroid (will add it to exclusion list)
19:16:06.11 +03:01:38.7 -- not an asteroid (will add it to exclusion list)
18:50:50.13 +07:08:32.8 -- not an asteroid (will add it to exclusion list)
19:15:25.06 +02:55:03.2 -- not an asteroid (will add it to exclusion list)
19:21:45.86 +04:41:40.7 -- not an asteroid (will add it to exclusion list)
19:17:17.07 +04:08:08.3 -- not an asteroid (will add it to exclusion list)
18:36:41.85 +09:56:19.7 -- not an asteroid (will add it to exclusion list)
18:24:33.20 +07:37:50.4 -- not an asteroid (will add it to exclusion list)
19:10:34.75 +01:41:13.0 -- not an asteroid (will add it to exclusion list)
19:15:00.22 +02:24:14.4 -- not an asteroid (will add it to exclusion list)
19:11:22.02 +01:34:33.5 -- not an asteroid (will add it to exclusion list)
19:11:11.94 +01:01:50.5 -- not an asteroid (will add it to exclusion list)
19:11:06.79 +00:53:52.5 -- not an asteroid (will add it to exclusion list)
19:13:39.05 +01:20:49.5 -- not an asteroid (will add it to exclusion list)
19:14:46.24 +02:14:58.2 -- not an asteroid (will add it to exclusion list)
19:10:33.22 +01:14:59.6 -- not an asteroid (will add it to exclusion list)
19:13:04.23 +02:15:36.6 -- not an asteroid (will add it to exclusion list)
18:22:02.19 +08:40:14.8 -- not an asteroid (will add it to exclusion list)
19:13:06.88 +01:32:11.9 -- not an asteroid (will add it to exclusion list)
19:12:49.69 +01:26:14.7 -- not an asteroid (will add it to exclusion list)
19:10:23.88 +01:29:27.3 -- not an asteroid (will add it to exclusion list)
18:38:03.01 +09:23:34.2 -- not an asteroid (will add it to exclusion list)
19:13:27.19 +01:53:34.7 -- not an asteroid (will add it to exclusion list)
19:17:48.87 +03:00:04.3 -- not an asteroid (will add it to exclusion list)
19:12:37.66 +02:43:00.2 -- not an asteroid (will add it to exclusion list)
19:12:13.89 +02:11:25.3 -- not an asteroid (will add it to exclusion list)
19:15:02.53 +02:19:30.8 -- not an asteroid (will add it to exclusion list)
19:15:50.62 +02:48:17.6 -- not an asteroid (will add it to exclusion list)
19:12:48.99 +01:02:31.4 -- not an asteroid (will add it to exclusion list)
18:23:41.32 +07:53:52.2 -- not an asteroid (will add it to exclusion list)
19:18:43.58 +03:12:54.7 -- not an asteroid (will add it to exclusion list)
19:08:34.97 +00:58:07.9 -- not an asteroid (will add it to exclusion list)
18:39:04.66 +09:01:25.9 -- not an asteroid (will add it to exclusion list)
19:18:33.71 +03:04:14.5 -- not an asteroid (will add it to exclusion list)
19:12:10.31 +01:05:15.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:22:02.19 +08:40:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:48.75 +08:35:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:23:41.32 +07:53:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:33.20 +07:37:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:48.12 +07:21:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:29:40.19 +07:38:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:30:20.44 +09:58:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:30:48.38 +08:01:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:34:15.36 +09:04:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:34:56.38 +08:10:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:35:40.81 +08:58:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:35:59.12 +09:27:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:36:18.15 +08:04:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:36:41.85 +09:56:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:36:44.34 +09:00:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:18.07 +09:11:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:18.10 +08:22:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:19.86 +07:47:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:51.03 +09:35:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:03.01 +09:23:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:25.02 +08:58:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:39:04.66 +09:01:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:39:14.92 +08:50:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:39:37.76 +09:03:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:58.07 +01:11:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:58.85 +10:41:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:50.13 +07:08:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:37.56 +05:21:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:31.32 +00:59:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:34.97 +00:58:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:42.78 +01:22:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:54.40 +01:19:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:55.77 +00:54:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:15.41 +01:05:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:22.42 +01:12:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:25.59 +01:00:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:40.50 +01:11:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:49.48 +01:25:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:52.82 +01:08:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:58.61 +01:40:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:18.03 +00:51:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:23.88 +01:29:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:33.22 +01:14:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:34.26 +00:53:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:34.75 +01:41:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:43.80 +01:16:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:45.87 +01:14:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:04.68 +01:56:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:06.79 +00:53:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:11.94 +01:01:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:13.06 +00:53:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:19.95 +01:47:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:22.02 +01:34:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:25.00 +01:44:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:31.35 +01:10:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:33.77 +01:05:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:37.11 +01:14:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:44.59 +01:09:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:49.26 +01:00:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:03.17 +01:14:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:04.74 +01:07:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:05.39 +02:21:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:06.38 +01:35:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:10.31 +01:05:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:13.89 +02:11:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:18.71 +02:33:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:20.36 +01:55:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:22.67 +01:00:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:22.99 +01:07:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:24.66 +01:12:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:33.70 +01:40:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:37.66 +02:43:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:38.61 +00:58:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:41.25 +02:15:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:45.60 +01:33:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:47.48 +01:23:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:48.43 +01:45:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:48.99 +01:02:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:49.69 +01:26:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:51.82 +01:36:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:54.83 +02:13:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:58.76 +01:51:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:04.23 +02:15:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:06.88 +01:32:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:12.33 +01:51:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:23.64 +01:52:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:27.19 +01:53:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:30.09 +02:25:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:39.05 +01:20:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:42.31 +01:59:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:43.37 +01:24:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:49.37 +02:21:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:50.94 +02:05:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:51.54 +02:07:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:06.44 +01:50:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:13.57 +02:11:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:21.38 +03:10:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:28.31 +02:02:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:38.84 +02:20:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:41.34 +02:36:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:42.73 +02:51:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:45.85 +02:21:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:46.24 +02:14:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:50.09 +02:31:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:00.22 +02:24:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:02.53 +02:19:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:05.00 +03:03:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:06.08 +02:06:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:07.67 +02:21:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:17.09 +02:11:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:20.01 +02:31:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:23.96 +03:00:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:25.06 +02:55:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:29.29 +02:19:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:31.50 +02:08:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:33.78 +02:27:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:35.37 +02:44:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:35.44 +02:49:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:41.66 +02:12:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:50.62 +02:48:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:51.47 +01:41:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:54.53 +02:44:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:59.03 +03:42:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:59.29 +03:28:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:59.79 +02:11:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:06.11 +03:01:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:08.18 +03:15:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:09.46 +02:41:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:17.63 +02:19:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:18.18 +03:24:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:19.17 +03:08:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:24.58 +02:44:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:28.64 +02:56:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:29.23 +02:43:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:31.51 +03:23:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:34.08 +03:27:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:36.52 +02:39:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:39.50 +02:20:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:43.76 +02:53:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:44.49 +02:32:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:59.69 +03:40:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:00.90 +03:03:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:03.27 +03:16:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:08.71 +02:53:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:17.07 +04:08:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:17.99 +03:18:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:25.72 +03:04:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:26.16 +03:19:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:48.87 +03:00:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:59.56 +03:41:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:32.77 +03:33:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:33.71 +03:04:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:43.58 +03:12:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:53.87 +04:17:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:05.82 +03:33:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:09.82 +03:22:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:09.96 +03:21:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:11.82 +03:42:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:24.42 +03:36:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:41.66 +04:23:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:37.79 +04:38:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:54.22 +04:24:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:58.87 +03:59:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:37.63 +05:20:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:45.03 +05:34:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:45.86 +04:41:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:48.79 +05:07:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:08.49 +05:45:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:12.56 +05:12:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:17.57 +05:43:17.0 -- 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)
18:22:02.19 +08:40:14.8 -- a known variable star
18:22:48.75 +08:35:49.3 -- a known variable star
18:23:41.32 +07:53:52.2 -- a known variable star
18:24:33.20 +07:37:50.4 -- a known variable star
18:28:48.12 +07:21:45.0 -- a known variable star
18:29:40.19 +07:38:22.2 -- a known variable star
18:30:20.44 +09:58:11.0 -- a known variable star
18:30:48.38 +08:01:23.0 -- a known variable star
18:34:15.36 +09:04:11.0 -- a known variable star
18:34:56.38 +08:10:00.6 -- a known variable star
18:35:40.81 +08:58:00.1 -- a known variable star
18:35:59.12 +09:27:39.2 -- a known variable star
18:36:18.15 +08:04:10.9 -- a known variable star
18:36:41.85 +09:56:19.7 -- a known variable star
18:36:44.34 +09:00:04.4 -- a known variable star
18:37:18.07 +09:11:21.6 -- a known variable star
18:37:18.10 +08:22:25.0 -- a known variable star
18:37:19.86 +07:47:43.9 -- a known variable star
18:37:51.03 +09:35:49.2 -- a known variable star
18:38:03.01 +09:23:34.2 -- a known variable star
18:38:25.02 +08:58:31.5 -- not a known variable star
18:39:04.66 +09:01:25.9 -- a known variable star
18:39:14.92 +08:50:13.6 -- not a known variable star
18:39:37.76 +09:03:36.6 -- not a known variable star
18:49:58.07 +01:11:11.3 -- a known variable star
18:49:58.85 +10:41:08.6 -- a known variable star
18:50:50.13 +07:08:32.8 -- a known variable star
18:51:37.56 +05:21:58.2 -- a known variable star
19:08:31.32 +00:59:05.4 -- a known variable star
19:08:34.97 +00:58:07.9 -- a known variable star
19:08:42.78 +01:22:46.1 -- a known variable star
19:08:54.40 +01:19:41.5 -- a known variable star
19:08:55.77 +00:54:57.0 -- a known variable star
19:09:15.41 +01:05:04.1 -- a known variable star
19:09:22.42 +01:12:15.4 -- a known variable star
19:09:25.59 +01:00:44.5 -- not a known variable star
19:09:40.50 +01:11:06.0 -- not a known variable star
19:09:49.48 +01:25:27.0 -- a known variable star
19:09:52.82 +01:08:27.6 -- not a known variable star
19:09:58.61 +01:40:52.7 -- a known variable star
19:10:18.03 +00:51:17.2 -- not a known variable star
19:10:23.88 +01:29:27.3 -- a known variable star
19:10:33.22 +01:14:59.6 -- a known variable star
19:10:34.26 +00:53:03.3 -- a known variable star
19:10:34.75 +01:41:13.0 -- a known variable star
19:10:43.80 +01:16:32.7 -- not a known variable star
19:10:45.87 +01:14:45.1 -- a known variable star
19:11:04.68 +01:56:12.2 -- not a known variable star
19:11:06.79 +00:53:52.5 -- not a known variable star
19:11:11.94 +01:01:50.5 -- a known variable star
19:11:13.06 +00:53:34.5 -- a known variable star
19:11:19.95 +01:47:21.7 -- not a known variable star
19:11:22.02 +01:34:33.5 -- not a known variable star
19:11:25.00 +01:44:06.8 -- a known variable star
19:11:31.35 +01:10:51.3 -- not a known variable star
19:11:33.77 +01:05:12.0 -- not a known variable star
19:11:37.11 +01:14:14.0 -- not a known variable star
19:11:44.59 +01:09:26.4 -- a known variable star
19:11:49.26 +01:00:08.6 -- a known variable star
19:12:03.17 +01:14:11.7 -- not a known variable star
19:12:04.74 +01:07:02.9 -- not a known variable star
19:12:05.39 +02:21:10.6 -- a known variable star
19:12:06.38 +01:35:19.2 -- not a known variable star
19:12:10.31 +01:05:15.9 -- a known variable star
19:12:13.89 +02:11:25.3 -- not a known variable star
19:12:18.71 +02:33:26.4 -- not a known variable star
19:12:20.36 +01:55:15.4 -- a known variable star
19:12:22.67 +01:00:55.9 -- a known variable star
19:12:22.99 +01:07:09.0 -- a known variable star
19:12:24.66 +01:12:47.1 -- not a known variable star
19:12:33.70 +01:40:10.4 -- a known variable star
19:12:37.66 +02:43:00.2 -- a known variable star
19:12:38.61 +00:58:49.9 -- not a known variable star
19:12:41.25 +02:15:06.7 -- not a known variable star
19:12:45.60 +01:33:22.1 -- not a known variable star
19:12:47.48 +01:23:15.5 -- a known variable star
19:12:48.43 +01:45:53.5 -- a known variable star
19:12:48.99 +01:02:31.4 -- a known variable star
19:12:49.69 +01:26:14.7 -- a known variable star
19:12:51.82 +01:36:07.5 -- a known variable star
19:12:54.83 +02:13:22.8 -- a known variable star
19:12:58.76 +01:51:37.3 -- not a known variable star
19:13:04.23 +02:15:36.6 -- not a known variable star
19:13:06.88 +01:32:11.9 -- not a known variable star
19:13:12.33 +01:51:04.7 -- not a known variable star
19:13:23.64 +01:52:46.4 -- not a known variable star
19:13:27.19 +01:53:34.7 -- a known variable star
19:13:30.09 +02:25:17.7 -- a known variable star
19:13:39.05 +01:20:49.5 -- a known variable star
19:13:42.31 +01:59:41.7 -- not a known variable star
19:13:43.37 +01:24:35.7 -- not a known variable star
19:13:49.37 +02:21:19.6 -- a known variable star
19:13:50.94 +02:05:11.8 -- not a known variable star
19:13:51.54 +02:07:15.2 -- a known variable star
19:14:06.44 +01:50:04.1 -- not a known variable star
19:14:13.57 +02:11:10.8 -- not a known variable star
19:14:21.38 +03:10:09.9 -- not a known variable star
19:14:28.31 +02:02:54.2 -- a known variable star
19:14:38.84 +02:20:08.6 -- a known variable star
19:14:41.34 +02:36:31.1 -- not a known variable star
19:14:42.73 +02:51:60.0 -- not a known variable star
19:14:45.85 +02:21:28.7 -- a known variable star
19:14:46.24 +02:14:58.2 -- not a known variable star
19:14:50.09 +02:31:41.3 -- not a known variable star
19:15:00.22 +02:24:14.4 -- not a known variable star
19:15:02.53 +02:19:30.8 -- not a known variable star
19:15:05.00 +03:03:55.6 -- not a known variable star
19:15:06.08 +02:06:40.6 -- not a known variable star
19:15:07.67 +02:21:22.9 -- not a known variable star
19:15:17.09 +02:11:14.3 -- not a known variable star
19:15:20.01 +02:31:03.6 -- not a known variable star
19:15:23.96 +03:00:51.4 -- a known variable star
19:15:25.06 +02:55:03.2 -- not a known variable star
19:15:29.29 +02:19:06.1 -- a known variable star
19:15:31.50 +02:08:35.3 -- a known variable star
19:15:33.78 +02:27:12.9 -- not a known variable star
19:15:35.37 +02:44:04.2 -- not a known variable star
19:15:35.44 +02:49:51.5 -- a known variable star
19:15:41.66 +02:12:58.8 -- a known variable star
19:15:50.62 +02:48:17.6 -- not a known variable star
19:15:51.47 +01:41:49.2 -- a known variable star
19:15:54.53 +02:44:55.9 -- not a known variable star
19:15:59.03 +03:42:28.9 -- a known variable star
19:15:59.29 +03:28:20.5 -- not a known variable star
19:15:59.79 +02:11:07.1 -- not a known variable star
19:16:06.11 +03:01:38.7 -- not a known variable star
19:16:08.18 +03:15:01.8 -- a known variable star
19:16:09.46 +02:41:47.4 -- not a known variable star
19:16:17.63 +02:19:17.0 -- a known variable star
19:16:18.18 +03:24:06.6 -- a known variable star
19:16:19.17 +03:08:18.3 -- not a known variable star
19:16:24.58 +02:44:49.4 -- not a known variable star
19:16:28.64 +02:56:23.9 -- not a known variable star
19:16:29.23 +02:43:12.5 -- not a known variable star
19:16:31.51 +03:23:26.8 -- not a known variable star
19:16:34.08 +03:27:26.8 -- a known variable star
19:16:36.52 +02:39:51.6 -- not a known variable star
19:16:39.50 +02:20:36.0 -- not a known variable star
19:16:43.76 +02:53:56.7 -- not a known variable star
19:16:44.49 +02:32:42.0 -- not a known variable star
19:16:59.69 +03:40:16.1 -- not a known variable star
19:17:00.90 +03:03:21.5 -- a known variable star
19:17:03.27 +03:16:34.1 -- not a known variable star
19:17:08.71 +02:53:14.9 -- a known variable star
19:17:17.07 +04:08:08.3 -- not a known variable star
19:17:17.99 +03:18:40.6 -- a known variable star
19:17:25.72 +03:04:12.4 -- not a known variable star
19:17:26.16 +03:19:46.5 -- a known variable star
19:17:48.87 +03:00:04.3 -- not a known variable star
19:17:59.56 +03:41:43.2 -- not a known variable star
19:18:32.77 +03:33:36.4 -- a known variable star
19:18:33.71 +03:04:14.5 -- a known variable star
19:18:43.58 +03:12:54.7 -- a known variable star
19:18:53.87 +04:17:35.9 -- a known variable star
19:19:05.82 +03:33:07.7 -- a known variable star
19:19:09.82 +03:22:01.2 -- a known variable star
19:19:09.96 +03:21:17.4 -- a known variable star
19:19:11.82 +03:42:32.2 -- not a known variable star
19:19:24.42 +03:36:24.1 -- not a known variable star
19:19:41.66 +04:23:22.6 -- a known variable star
19:20:37.79 +04:38:35.2 -- a known variable star
19:20:54.22 +04:24:59.7 -- a known variable star
19:20:58.87 +03:59:47.1 -- a known variable star
19:21:37.63 +05:20:33.3 -- a known variable star
19:21:45.03 +05:34:08.4 -- a known variable star
19:21:45.86 +04:41:40.7 -- a known variable star
19:21:48.79 +05:07:49.7 -- not a known variable star
19:22:08.49 +05:45:50.9 -- not a known variable star
19:22:12.56 +05:12:55.4 -- a known variable star
19:22:17.57 +05:43:17.0 -- a known variable star
Found 74 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
170 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 170 (excluding asteroids and hot pixels, 74 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461186.70096229 -observatory V36
05:07:21.46 +24:43:30.1 Mercury (-1.1mag)
06:35:59.75 +24:58:56.6 Venus (-3.9mag)
02:12:06.19 +12:34:08.3 Mars (1.3mag)
07:37:59.95 +21:56:23.9 Jupiter (-1.9mag)
00:45:18.39 +02:25:55.0 Saturn (0.9mag)
03:57:04.40 +20:16:19.6 Uranus (5.8mag)
00:15:13.81 +00:11:34.2 Neptune (7.8mag)
20:33:56.24 -23:00:04.1 Pluto (14.5mag)
12:20:14.83 -05:52:35.6 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 25 23:52 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461186.70096229:
07:37:54.95 +21:56:36.5 Io (5.9mag)
07:38:10.40 +21:55:54.1 Europa (6.1mag)
07:37:53.00 +21:56:48.2 Ganymede (5.5mag)
07:37:38.09 +21:57:17.4 Callisto (6.7mag)
07:39:05.00 +21:32:44.4 Himalia (15.5mag)
07:38:00.71 +21:56:23.2 Thebe (16.5mag)
07:39:23.34 +21:53:59.4 Elara (17.5mag)
07:39:27.80 +22:15:08.5 Pasiphae (17.7mag)
07:45:07.03 +21:57:13.5 Carme (18.8mag)
00:45:20.59 +02:25:35.2 Titan (8.7mag)
00:45:14.37 +02:26:02.7 Rhea (10.0mag)
00:45:41.10 +02:26:01.9 Iapetus (11.4mag)
00:45:33.12 +02:25:57.9 Hyperion (14.7mag)
00:46:16.01 +02:29:41.8 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 23:52 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.70096229:
17:17:22.68 -33:20:57.6 JWST
16:05:14.42 +52:06:15.7 Chandra
08:21:37.43 -45:14:35.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 23:52 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.70096229 -observatory V36
13:20:46.00 -27:03:30.4 14.4mag D/1884 O1 (Barnard)
06:37:24.21 +30:40:17.6 15.7mag D/1886 K1 (Brooks)
15:26:16.68 +01:21:00.5 14.6mag D/1895 Q1 (Swift)
05:28:12.48 +24:38:56.9 17.2mag D/1918 W1 (Schorr)
09:31:29.89 +14:31:48.4 17.9mag P/2009 WX51 (Catalina)
18:51:00.56 -31:39:31.2 13.7mag P/2010 H2 (Vales)
05:40:54.08 -68:16:01.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:21.73 +31:48:30.8 17.4mag C/2017 K2 (PANSTARRS)
17:19:51.26 +14:33:01.3 17.7mag C/2021 G2 (ATLAS)
23:14:32.77 +31:02:52.4 17.2mag C/2022 E2 (ATLAS)
05:18:01.94 +26:51:29.3 16.4mag C/2022 N2 (PANSTARRS)
09:20:58.48 +31:29:34.3 16.5mag C/2022 QE78 (ATLAS)
08:44:01.62 +03:13:10.6 17.6mag C/2022 R6 (PANSTARRS)
18:36:21.05 +21:12:19.5 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:26.52 -11:02:15.9 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.46 +65:39:50.2 17.7mag C/2023 H5 (Lemmon)
18:17:03.65 -05:32:14.7 13.7mag C/2023 R1 (PANSTARRS)
13:39:44.13 +85:47:48.7 17.9mag C/2023 X2 (Lemmon)
06:53:27.42 +63:55:43.9 17.6mag C/2024 A1 (ATLAS)
06:26:55.05 +26:29:01.6 13.1mag C/2024 E1 (Wierzchos)
15:47:52.04 +12:12:40.5 17.3mag C/2024 G6 (ATLAS)
20:19:47.49 +27:10:47.7 14.1mag C/2024 J3 (ATLAS)
04:05:00.08 -17:12:07.6 16.1mag C/2024 T5 (ATLAS)
05:53:40.67 +36:48:41.6 17.9mag C/2025 J1 (Borisov)
11:45:40.20 +53:20:10.8 16.9mag C/2025 L1 (ATLAS)
06:24:57.58 -10:11:22.5 12.6mag C/2025 R3 (PANSTARRS)
12:40:57.01 +04:37:00.1 17.2mag C/2025 Y1 (ATLAS)
01:36:21.28 +42:23:02.2 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.43 -08:58:44.5 16.3mag A/2026 E1
19:59:42.29 -08:07:25.5 9.5mag 10P/Tempel
14:18:44.93 -02:35:34.4 17.6mag 24P/Schaumasse
10:59:43.28 -00:51:55.2 15.9mag 29P/Schwassmann-Wachmann
10:51:19.92 -02:34:28.7 17.8mag 43P/Wolf-Harrington
02:51:29.40 +23:50:19.7 17.6mag 47P/Ashbrook-Jackson
08:32:17.17 +27:21:47.7 16.9mag 63P/Wild
00:14:54.22 -07:19:14.5 15.7mag 65P/Gunn
06:01:42.20 +31:41:18.2 16.5mag 76P/West-Kohoutek-Ikemura
02:38:00.60 +15:23:35.6 13.9mag 78P/Gehrels
00:51:11.89 +01:49:27.9 15.3mag 88P/Howell
04:12:49.97 +28:56:49.7 15.1mag 93P/Lovas
02:07:27.98 +25:21:24.7 17.9mag 114P/Wiseman-Skiff
06:20:02.27 +33:19:27.0 15.7mag 123P/West-Hartley
09:27:59.34 +20:15:39.2 16.4mag 124P/Mrkos
03:37:38.06 +18:17:27.2 16.4mag 128P/Shoemaker-Holt
04:07:36.60 +18:20:58.6 17.7mag 131P/Mueller
04:58:47.70 +19:38:40.2 13.0mag 141P/Machholz
05:01:26.37 +16:23:05.7 12.9mag 141P-A/Machholz
03:46:37.13 +13:43:21.9 10.6mag 141P-D/Machholz
02:48:12.71 -26:39:02.0 17.3mag 161P/Hartley-IRAS
02:59:57.55 +18:14:28.3 14.9mag 162P/SidingSpring
19:34:45.33 -01:42:24.7 17.6mag 169P/NEAT
17:02:20.41 -09:21:26.7 16.2mag 235P/LINEAR
07:05:04.61 +35:51:51.6 17.3mag 240P/NEAT
23:58:36.15 -07:45:47.4 16.7mag 260P/McNaught
03:30:03.13 +29:55:36.2 17.7mag 295P/LINEAR
22:05:26.21 -27:28:59.0 17.7mag 320P/McNaught
15:21:44.14 +08:21:36.7 17.4mag 391P/Kowalski
07:57:13.99 +21:02:17.7 17.8mag 450P/LONEOS
06:38:47.33 +42:35:09.9 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 23:52 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
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
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 25 23:52 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 25 23:52 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:51:00.147 -40:59:30.34 AT 2026myv 2026-05-04.40 19.85
23:01:42.557 -37:41:28.08 AT 2026myu 2026-05-14.36 20.03
17:40:41.796 +55:46:35.59 AT 2026myt 2026-05-13.08 19.76
11:57:21.623 +08:17:50.60 AT 2026mys 2026-05-17.92 20.12
18:08:09.175 +24:46:16.68 AT 2026myr 2026-05-16.11 19.59
19:44:08.720 +05:58:44.85 AT 2026myq 2026-05-18.09 19.96
22:15:03.694 +37:18:03.97 SN 2026myp 2026-05-17.58 17.878
13:28:54.990 -05:49:13.50 AT 2026myo 2026-05-17.76 18.69
13:35:39.060 +60:25:07.59 AT 2026myn 2026-05-17.79 18.94
15:11:37.375 +27:04:22.10 AT 2026mym 2026-05-17.80 19.01
15:45:32.128 +08:10:41.12 AT 2026myl 2026-05-17.84 19.27
16:38:47.743 +40:50:56.52 AT 2026myk 2026-05-17.88 18.14
13:21:16.033 -33:01:10.62 AT 2026myj 2026-05-10.44 20.34
14:04:07.440 +19:21:36.43 AT 2026myi 2026-05-16.96 20.28
12:09:08.262 +13:15:11.92 AT 2026myh 2026-05-05.92 20.33
17:37:21.286 +36:24:32.57 AT 2026myg 2026-05-12.55 19.89
14:40:52.425 +10:22:25.10 AT 2026myf 2026-05-14.32 20.45
21:41:13.013 +64:08:54.76 AT 2026mye 2026-05-17.15 19.242
17:07:33.400 +35:38:40.42 AT 2026myd 2026-05-17.43 20.44
20:38:48.864 -58:53:21.28 AT 2026myc 2026-05-13.27 19.093
-rw-r--r-- 1 apache apache 30K May 25 23:52 tns_transients_list.txt
