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-Q2b1x1_234857_TTUQ2b1x1_2017996_3sLqWVBV
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 26.1984 2461186.6984 11.20 19:08:12.89 +02:21:06.3
36.94111 -2.65523 galactic Aql Second-epoch detections are separated by 2.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.0547+02.3515 | 19:08:13.15 +02:21:05.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:12.89 +02:21:06.3: 12.45 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:12.89 +02:21:06.3: 12.52 +/- 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
ATO J287.0547+02.3515,2461186.6984,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0547+02.3515 20260526.1984 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.99 19:07:22.39 +02:37:13.5
37.08354 -2.34519 galactic Aql Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8436+02.6202 | 19:07:22.48 +02:37:13.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M3 1964AbaOB..31...27A [A64] Red +02 114 J-Ks=1.345+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:22.39 +02:37:13.5: 12.11 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:22.39 +02:37:13.5: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 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 J286.8436+02.6202,2461186.6984,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8436+02.6202 20260526.1984 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 26.1984 2461186.6984 11.70 19:06:23.35 +01:56:28.2
36.36656 -2.43810 galactic Aql Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.5856+01.9471 | 19:06:23.35 +01:56:28.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.357+/-0.031 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:23.35 +01:56:28.2: 12.98 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:23.35 +01:56:28.2: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 J286.5856+01.9471,2461186.6984,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.5856+01.9471 20260526.1984 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.79 19:06:47.96 +02:08:43.7
36.59532 -2.43558 galactic Aql Second-epoch detections are separated by 1.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:06:47.96 +02:08:43.7 (user input) | T | P | (position from user input) J-Ks=0.711+/-0.043 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:47.96 +02:08:43.7: 13.21 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:47.96 +02:08:43.7: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6984,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.1984 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.60 18:43:36.35 +02:04:16.7
33.88397 2.68640 galactic Aql Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4278947312810200192 | 18:43:36.31 +02:04:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:43:36.35 +02:04:16.7: 12.53 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:43:36.35 +02:04:16.7: 12.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 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 4278947312810200192,2461186.6984,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4278947312810200192 20260526.1984 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 26.1984 2461186.6984 11.72 19:08:59.41 +02:20:11.8
37.01662 -2.83426 galactic Aql Second-epoch detections are separated by 1.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.2499+02.3363 | 19:08:59.41 +02:20:11.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.782+/-0.038 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:59.41 +02:20:11.8: 13.06 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:59.41 +02:20:11.8: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.06 +/- 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
ATO J287.2499+02.3363,2461186.6984,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.2499+02.3363 20260526.1984 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.64 19:05:59.00 +01:56:09.7
36.31550 -2.35032 galactic Aql Second-epoch detections are separated by 3.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267684774731121664 | 19:05:59.03 +01:56:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.822+/-0.035 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:59.00 +01:56:09.7: 12.82 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:59.00 +01:56:09.7: 12.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 4267684774731121664,2461186.6984,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267684774731121664 20260526.1984 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 26.1984 2461186.6984 11.43 19:07:39.68 +02:11:07.2
36.72959 -2.60869 galactic Aql Second-epoch detections are separated by 3.6" and 6.0 pix
The object was found in VSX 2" Gaia DR3 4267715831592269056
Type: ROT
# Max. Min./Amp. JD0 Period
12.330 G 12.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:39.68 +02:11:07.2: 12.57 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:39.68 +02:11:07.2: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 4267715831592269056,2461186.6984,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267715831592269056 20260526.1984 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.21 19:07:25.90 +02:35:57.3
37.07143 -2.36788 galactic Aql Second-epoch detections are separated by 1.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268857330820916096 | 19:07:25.97 +02:35:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +02 115 J-Ks=1.133+/-0.028 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:25.90 +02:35:57.3: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:25.90 +02:35:57.3: 12.27 +/- 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 4268857330820916096,2461186.6984,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268857330820916096 20260526.1984 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 26.1984 2461186.6984 11.21 19:07:26.74 +02:14:39.4
36.75730 -2.53378 galactic Aql Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267719924745168768 | 19:07:26.67 +02:14:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.145+/-0.035 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:26.74 +02:14:39.4: 12.30 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:26.74 +02:14:39.4: 12.37 +/- 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 4267719924745168768,2461186.6984,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267719924745168768 20260526.1984 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 26.1984 2461186.6984 10.80 19:06:40.69 +02:02:59.1
36.49628 -2.45254 galactic Aql Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6574+02.0524 | 19:06:40.73 +02:02:58.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.856+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:40.69 +02:02:59.1: 11.89 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:40.69 +02:02:59.1: 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
ATO J286.6574+02.0524,2461186.6984,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6574+02.0524 20260526.1984 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 26.1984 2461186.6984 11.71 19:06:10.29 +02:03:04.0
36.43944 -2.33940 galactic Aql Second-epoch detections are separated by 2.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267688068923662720 | 19:06:10.31 +02:03:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.787+/-0.032 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:10.29 +02:03:04.0: 12.90 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:10.29 +02:03:04.0: 12.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 4267688068923662720,2461186.6984,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267688068923662720 20260526.1984 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 26.1984 2461186.6984 11.57 19:08:05.19 +02:16:24.4
36.85674 -2.66266 galactic Aql Second-epoch detections are separated by 3.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:08:05.19 +02:16:24.4 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.055 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:05.19 +02:16:24.4: 12.67 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:05.19 +02:16:24.4: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6984,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.1984 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 26.1984 2461186.6984 11.68 19:08:45.19 +02:40:45.7
37.29427 -2.62434 galactic Aql Second-epoch detections are separated by 2.9" and 5.1 pix
The object was found in VSX20" Gaia DR3 4268861252182520832
Type: E
# Max. Min./Amp. JD0 Period
16.080 G 17.050 G 2.919530000000 B
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:45.19 +02:40:45.7: 12.97 +/- 0.04 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:45.19 +02:40:45.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.97 +/- 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
Gaia DR3 4268861252182520832,2461186.6984,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268861252182520832 20260526.1984 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.63 19:06:25.40 +01:59:40.2
36.41793 -2.42126 galactic Aql Second-epoch detections are separated by 3.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267683945755060224 | 19:06:25.48 +01:59:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.882+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:25.40 +01:59:40.2: 12.96 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:25.40 +01:59:40.2: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 4267683945755060224,2461186.6984,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267683945755060224 20260526.1984 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 26.1984 2461186.6984 11.44 19:07:20.99 +02:15:05.5
36.75276 -2.50918 galactic Aql Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267720160919295488 | 19:07:20.94 +02:15:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.267+/-0.033 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:20.99 +02:15:05.5: 12.40 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:20.99 +02:15:05.5: 12.66 +/- 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 4267720160919295488,2461186.6984,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267720160919295488 20260526.1984 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 26.1984 2461186.6984 11.38 19:07:53.71 +02:43:38.3
37.23846 -2.41197 galactic Aql Second-epoch detections are separated by 1.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9692+02.7261 | 19:07:53.77 +02:43:40.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.033 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:53.71 +02:43:38.3: 12.43 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:53.71 +02:43:38.3: 12.55 +/- 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
ATO J286.9692+02.7261,2461186.6984,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9692+02.7261 20260526.1984 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 26.1984 2461186.6984 11.57 19:07:19.21 +02:08:06.2
36.64575 -2.55599 galactic Aql Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8352+02.1396 | 19:07:19.18 +02:08:05.6 (Gaia DR3) | MSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.531+/-0.035 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:19.21 +02:08:06.2: 12.65 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:19.21 +02:08:06.2: 12.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 J286.8352+02.1396,2461186.6984,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8352+02.1396 20260526.1984 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 26.1984 2461186.6984 10.78 19:07:52.14 +01:55:20.3
36.51939 -2.77539 galactic Aql Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9657+01.9313 | 19:07:52.13 +01:55:19.3 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +01 101 J-Ks=1.130+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:52.14 +01:55:20.3: 11.98 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:52.14 +01:55:20.3: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.99 +/- 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 J286.9657+01.9313,2461186.6984,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9657+01.9313 20260526.1984 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 26.1984 2461186.6984 11.47 19:08:02.39 +02:20:34.3
36.91313 -2.62047 galactic Aql Second-epoch detections are separated by 4.1" and 6.1 pix
The object was found in VSX14" ZTF J190803.23+022041.2
Type: SR
# Max. Min./Amp. JD0 Period
15.165 r Y 1.223 r 2458293.40700 208.122280100000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:02.39 +02:20:34.3: 12.65 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:02.39 +02:20:34.3: 12.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 J190803.23+022041.2,2461186.6984,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190803.23+022041.2 20260526.1984 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 26.1984 2461186.6984 11.52 19:08:11.23 +02:44:50.7
37.28984 -2.46753 galactic Aql Second-epoch detections are separated by 1.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:08:11.23 +02:44:50.7 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.038 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:11.23 +02:44:50.7: 12.67 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:11.23 +02:44:50.7: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6984,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.1984 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 26.1984 2461186.6984 11.56 19:08:01.58 +03:04:56.0
37.56909 -2.27815 galactic Aql Second-epoch detections are separated by 3.4" and 5.7 pix
The object was found in VSX 1" ZTF J190801.57+030455.0
Type: RS
# Max. Min./Amp. JD0 Period
13.964 g Y 0.106 g 2458640.87930 10.196015800000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:01.58 +03:04:56.0: 12.68 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:01.58 +03:04:56.0: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 J190801.57+030455.0,2461186.6984,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190801.57+030455.0 20260526.1984 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 26.1984 2461186.6984 11.15 19:08:11.46 +02:05:51.0
36.71220 -2.76656 galactic Aql Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267703810027157248 | 19:08:11.47 +02:05:50.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:11.46 +02:05:51.0: 12.39 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:11.46 +02:05:51.0: 12.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 4267703810027157248,2461186.6984,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267703810027157248 20260526.1984 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 26.1984 2461186.6984 11.34 19:06:43.12 +02:28:57.5
36.88598 -2.26311 galactic Aql Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6823+02.4821 | 19:06:43.10 +02:28:58.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.030 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:43.12 +02:28:57.5: 12.39 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:43.12 +02:28:57.5: 12.53 +/- 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
ATO J286.6823+02.4821,2461186.6984,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6823+02.4821 20260526.1984 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 26.1984 2461186.6984 11.62 19:06:39.57 +02:24:16.7
36.80983 -2.28574 galactic Aql Second-epoch detections are separated by 1.9" and 5.2 pix
The object was found in VSX17" Gaia DR3 4268476663579757952
Type: L
# Max. Min./Amp. JD0 Period
18.610 G 19.110 G
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:39.57 +02:24:16.7: 12.65 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:39.57 +02:24:16.7: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4268476663579757952,2461186.6984,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268476663579757952 20260526.1984 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 26.1984 2461186.6984 10.13 19:07:38.10 +02:03:28.3
36.61317 -2.66129 galactic Aql Second-epoch detections are separated by 0.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9014+02.0569 | 19:07:38.12 +02:03:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.753+/-0.029 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:38.10 +02:03:28.3: 11.09 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:38.10 +02:03:28.3: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.11 +/- 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 J286.9014+02.0569,2461186.6984,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9014+02.0569 20260526.1984 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.95 19:08:13.69 +02:33:15.2
37.12273 -2.56529 galactic Aql Second-epoch detections are separated by 0.4" and 5.4 pix
The object was found in VSX 0" ASASSN-V J190813.70+023314.9
Type: DSCT
# Max. Min./Amp. JD0 Period
11.970 V 12.030 V 2457877.97800 0.112621000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:13.69 +02:33:15.2: 11.94 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:13.69 +02:33:15.2: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.96 +/- 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 J190813.70+023314.9,2461186.6984,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190813.70+023314.9 20260526.1984 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 26.1984 2461186.6984 11.29 19:07:45.47 +01:59:16.1
36.56493 -2.72068 galactic Aql Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267692638768872704 | 19:07:45.44 +01:59:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.856+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:45.47 +01:59:16.1: 12.67 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:45.47 +01:59:16.1: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 4267692638768872704,2461186.6984,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267692638768872704 20260526.1984 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 26.1984 2461186.6984 11.71 19:07:11.28 +02:37:34.2
37.06743 -2.30146 galactic Aql Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268869322369606144 | 19:07:11.23 +02:37:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.796+/-0.033 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:11.28 +02:37:34.2: 12.93 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:11.28 +02:37:34.2: 12.97 +/- 0.05 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
Gaia DR3 4268869322369606144,2461186.6984,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268869322369606144 20260526.1984 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 26.1984 2461186.6984 11.39 19:07:31.91 +02:47:51.9
37.25943 -2.29904 galactic Aql Second-epoch detections are separated by 2.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268877744856647936 | 19:07:31.81 +02:47:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.196+/-0.038 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:31.91 +02:47:51.9: 12.38 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:31.91 +02:47:51.9: 12.54 +/- 0.03 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
Gaia DR3 4268877744856647936,2461186.6984,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268877744856647936 20260526.1984 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 26.1984 2461186.6984 11.30 19:05:44.82 +02:02:31.9
36.38289 -2.24921 galactic Aql Second-epoch detections are separated by 0.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.4287+02.0485 | 19:05:44.88 +02:02:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.989+/-0.032 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:44.82 +02:02:31.9: 12.37 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:44.82 +02:02:31.9: 12.44 +/- 0.03 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
ATO J286.4287+02.0485,2461186.6984,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.4287+02.0485 20260526.1984 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.40 19:07:38.28 +03:00:46.9
37.46303 -2.22379 galactic Aql Second-epoch detections are separated by 1.3" and 5.7 pix
The object was found in VSX 1" Gaia DR3 4268908286313887488
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.130 G 12.180 G A
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:38.28 +03:00:46.9: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:38.28 +03:00:46.9: 12.46 +/- 0.03 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
Gaia DR3 4268908286313887488,2461186.6984,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268908286313887488 20260526.1984 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 26.1984 2461186.6984 11.34 19:06:42.67 +02:20:52.3
36.76525 -2.32324 galactic Aql Second-epoch detections are separated by 1.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268473188944297728 | 19:06:42.58 +02:20:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.049 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:42.67 +02:20:52.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:42.67 +02:20:52.3: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 4268473188944297728,2461186.6984,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268473188944297728 20260526.1984 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 26.1984 2461186.6984 11.49 19:07:38.79 +02:32:39.1
37.04710 -2.44081 galactic Aql Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268853104573101312 | 19:07:37.78 +02:32:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.032 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:38.79 +02:32:39.1: 12.62 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:38.79 +02:32:39.1: 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
Gaia DR3 4268853104573101312,2461186.6984,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268853104573101312 20260526.1984 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 26.1984 2461186.6984 11.04 19:07:20.69 +02:02:18.1
36.56255 -2.60580 galactic Aql Second-epoch detections are separated by 1.8" and 5.1 pix
The object was found in VSX 3" NSVS 14033079
Type: L
# Max. Min./Amp. JD0 Period
11.040 R1 Y 0.140 R1 M3
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:20.69 +02:02:18.1: 12.35 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:20.69 +02:02:18.1: 12.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 14033079,2461186.6984,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 14033079 20260526.1984 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 26.1984 2461186.6984 11.49 19:07:47.68 +02:02:07.7
36.61156 -2.70700 galactic Aql Second-epoch detections are separated by 2.9" and 5.7 pix
The object was found in VSX 2" ASASSN-V J190747.65+020206.2
Type: ROT
# Max. Min./Amp. JD0 Period
12.920 V 13.130 V 2457939.89800 35.090000000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:47.68 +02:02:07.7: 12.63 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:47.68 +02:02:07.7: 12.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 J190747.65+020206.2,2461186.6984,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190747.65+020206.2 20260526.1984 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 26.1984 2461186.6984 10.94 19:07:59.70 +03:16:25.6
37.73579 -2.18324 galactic Aql Second-epoch detections are separated by 1.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268968901251391616 | 19:07:59.78 +03:16:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 1964AbaOB..31...27A [A64] Red +03 98 J-Ks=1.199+/-0.036 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:59.70 +03:16:25.6: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:59.70 +03:16:25.6: 11.97 +/- 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
Gaia DR3 4268968901251391616,2461186.6984,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268968901251391616 20260526.1984 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 26.1984 2461186.6984 11.33 19:08:04.13 +03:04:09.4
37.56245 -2.29352 galactic Aql Second-epoch detections are separated by 1.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268910382257926912 | 19:08:04.15 +03:04:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1964AbaOB..31...27A [A64] Red +02 124 J-Ks=0.885+/-0.033 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:04.13 +03:04:09.4: 12.35 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:04.13 +03:04:09.4: 12.37 +/- 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
Gaia DR3 4268910382257926912,2461186.6984,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268910382257926912 20260526.1984 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.01 19:07:32.99 +02:13:42.1
36.75509 -2.56421 galactic Aql Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8951+02.2279 | 19:07:33.05 +02:13:41.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K5 1947AnDea...5....1L DO 5354 J-Ks=1.127+/-0.031 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:32.99 +02:13:42.1: 11.01 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:32.99 +02:13:42.1: 11.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J286.8951+02.2279,2461186.6984,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8951+02.2279 20260526.1984 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.71 19:07:55.27 +02:02:15.1
36.62789 -2.73415 galactic Aql Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267701748443856128 | 19:07:55.27 +02:02:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.434+/-0.029 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:55.27 +02:02:15.1: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:55.27 +02:02:15.1: 11.96 +/- 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
Gaia DR3 4267701748443856128,2461186.6984,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267701748443856128 20260526.1984 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 26.1984 2461186.6984 10.76 19:07:48.23 +01:56:29.2
36.52895 -2.75214 galactic Aql Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX 9" Gaia DR3 4267691882854110592
Type: E
# Max. Min./Amp. JD0 Period
18.050 G 18.220 G 1.003610000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:48.23 +01:56:29.2: 11.84 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:48.23 +01:56:29.2: 11.90 +/- 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 4267691882854110592,2461186.6984,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267691882854110592 20260526.1984 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 26.1984 2461186.6984 10.87 19:06:21.96 +02:18:10.7
36.68577 -2.26718 galactic Aql Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6018+02.3106 | 19:06:22.00 +02:18:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K5 1964AbaOB..31...27A [A64] Red +02 97 J-Ks=0.878+/-0.031 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:21.96 +02:18:10.7: 11.84 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:21.96 +02:18:10.7: 11.98 +/- 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
ATO J286.6018+02.3106,2461186.6984,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6018+02.3106 20260526.1984 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 26.1984 2461186.6984 11.32 19:05:50.36 +01:52:58.5
36.25176 -2.34266 galactic Aql Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.4474+01.8830 | 19:05:50.34 +01:52:57.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.875+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:50.36 +01:52:58.5: 12.34 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:50.36 +01:52:58.5: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 J286.4474+01.8830,2461186.6984,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.4474+01.8830 20260526.1984 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 26.1984 2461186.6984 10.03 19:07:42.37 +01:47:57.2
36.39120 -2.79564 galactic Aql Second-epoch detections are separated by 0.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9369+01.7975 | 19:07:42.43 +01:47:58.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:42.37 +01:47:57.2: 10.99 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:42.37 +01:47:57.2: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.02 +/- 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
ATO J286.9369+01.7975,2461186.6984,10.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9369+01.7975 20260526.1984 10.03CV 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 26.1984 2461186.6984 10.79 19:08:24.18 +02:53:37.2
37.44465 -2.44826 galactic Aql Second-epoch detections are separated by 2.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268902857467516032 | 19:08:24.11 +02:53:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.805+/-0.033 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:24.18 +02:53:37.2: 11.83 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:24.18 +02:53:37.2: 11.92 +/- 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 4268902857467516032,2461186.6984,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268902857467516032 20260526.1984 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 26.1984 2461186.6984 10.87 19:07:09.43 +02:21:50.5
36.83075 -2.41483 galactic Aql Second-epoch detections are separated by 0.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268473880469029376 | 19:07:09.37 +02:21:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.221+/-0.031 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:09.43 +02:21:50.5: 11.82 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:09.43 +02:21:50.5: 11.92 +/- 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
Gaia DR3 4268473880469029376,2461186.6984,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268473880469029376 20260526.1984 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 26.1984 2461186.6984 11.16 19:07:48.68 +02:01:05.7
36.59815 -2.71860 galactic Aql Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267695735488632576 | 19:07:48.73 +02:01:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.822+/-0.033 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:48.68 +02:01:05.7: 12.30 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:48.68 +02:01:05.7: 12.44 +/- 0.03 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
Gaia DR3 4267695735488632576,2461186.6984,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267695735488632576 20260526.1984 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 26.1984 2461186.6984 9.98 19:06:42.55 +01:50:48.7
36.31932 -2.55238 galactic Aql Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6845+01.8500 | 19:06:42.56 +01:50:48.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.878+/-0.028 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:42.55 +01:50:48.7: 10.88 +/- 0.00 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:42.55 +01:50:48.7: 10.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J286.6845+01.8500,2461186.6984,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6845+01.8500 20260526.1984 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.22 19:05:20.75 +01:50:52.0
36.16398 -2.24913 galactic Aql Second-epoch detections are separated by 1.3" and 5.3 pix
The object was found in VSX24" Gaia DR3 4267677898444876800
Type: YSO
# Max. Min./Amp. JD0 Period
17.030 G 17.190 G M
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:20.75 +01:50:52.0: 12.32 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:20.75 +01:50:52.0: 12.40 +/- 0.03 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
Gaia DR3 4267677898444876800,2461186.6984,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267677898444876800 20260526.1984 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 26.1984 2461186.6984 11.35 19:08:33.03 +02:46:56.7
37.36265 -2.53206 galactic Aql Second-epoch detections are separated by 1.3" and 5.3 pix
The object was found in VSX19" Gaia DR3 4268889186651882496
Type: L
# Max. Min./Amp. JD0 Period
13.760 G 13.900 G M
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:33.03 +02:46:56.7: 12.31 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:33.03 +02:46:56.7: 99.00 +/- 99.00 bad_region
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
Gaia DR3 4268889186651882496,2461186.6984,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268889186651882496 20260526.1984 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 26.1984 2461186.6984 11.35 19:05:20.25 +01:52:13.2
36.18310 -2.23695 galactic Aql Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267678693056773120 | 19:05:20.22 +01:52:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.247+/-0.031 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:20.25 +01:52:13.2: 12.30 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:20.25 +01:52:13.2: 12.48 +/- 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 4267678693056773120,2461186.6984,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267678693056773120 20260526.1984 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 26.1984 2461186.6984 11.13 19:07:32.71 +01:50:08.0
36.40507 -2.74323 galactic Aql Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8726+01.8282 | 19:07:31.35 +01:49:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.891+/-0.033 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:32.71 +01:50:08.0: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:32.71 +01:50:08.0: 12.39 +/- 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 J286.8726+01.8282,2461186.6984,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8726+01.8282 20260526.1984 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.24 19:06:46.38 +02:04:19.6
36.52704 -2.46335 galactic Aql Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267708139354812800 | 19:06:46.45 +02:04:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +01 82 J-Ks=1.161+/-0.031 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:46.38 +02:04:19.6: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:46.38 +02:04:19.6: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.31 +/- 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 4267708139354812800,2461186.6984,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267708139354812800 20260526.1984 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 26.1984 2461186.6984 11.21 19:07:40.86 +02:47:19.4
37.26851 -2.33627 galactic Aql Second-epoch detections are separated by 0.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268876954582617344 | 19:07:40.81 +02:47:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +02 120 J-Ks=1.035+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:40.86 +02:47:19.4: 12.31 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:40.86 +02:47:19.4: 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
Gaia DR3 4268876954582617344,2461186.6984,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268876954582617344 20260526.1984 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 26.1984 2461186.6984 10.77 19:05:51.10 +01:56:43.4
36.30875 -2.31679 galactic Aql Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267684946529836928 | 19:05:51.13 +01:56:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 1964AbaOB..31...27A [A64] Red +01 73 J-Ks=1.247+/-0.026 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:51.10 +01:56:43.4: 11.80 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:51.10 +01:56:43.4: 11.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.81 +/- 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 4267684946529836928,2461186.6984,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267684946529836928 20260526.1984 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.85 19:06:46.37 +02:16:28.1
36.70704 -2.37057 galactic Aql Second-epoch detections are separated by 0.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268471578366534528 | 19:06:46.51 +02:16:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +02 106 J-Ks=1.105+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:46.37 +02:16:28.1: 11.81 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:46.37 +02:16:28.1: 11.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.84 +/- 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 4268471578366534528,2461186.6984,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268471578366534528 20260526.1984 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.24 19:08:31.82 +02:19:12.8
36.94927 -2.73972 galactic Aql Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.1285+02.3153 | 19:08:31.90 +02:19:14.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:31.82 +02:19:12.8: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:31.82 +02:19:12.8: 99.00 +/- 99.00 bad_region
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
ATO J287.1285+02.3153,2461186.6984,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1285+02.3153 20260526.1984 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 26.1984 2461186.6984 11.66 18:42:50.40 +02:11:29.7
33.90405 2.91150 galactic Ser Second-epoch detections are separated by 0.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4279703600705323776 | 18:42:50.43 +02:11:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.621+/-0.032 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 18:42:50.40 +02:11:29.7: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 18:42:50.40 +02:11:29.7: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 26.1984* 18 42 50.40 +02 11 29.7 11.7 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
Gaia DR3 4279703600705323776,2461186.6984,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4279703600705323776 20260526.1984 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 26.1984 2461186.6984 11.41 19:06:48.29 +01:53:15.3
36.36651 -2.55497 galactic Aql Second-epoch detections are separated by 1.1" and 5.5 pix
The object was found in VSX 6" Gaia DR3 4267670378000335360
Type: L
# Max. Min./Amp. JD0 Period
16.070 G 16.210 G M
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:48.29 +01:53:15.3: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:48.29 +01:53:15.3: 12.78 +/- 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 4267670378000335360,2461186.6984,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267670378000335360 20260526.1984 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 26.1984 2461186.6984 11.41 19:05:56.45 +02:17:18.9
36.62426 -2.17937 galactic Aql Second-epoch detections are separated by 2.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268470165287324416 | 19:05:56.49 +02:17:18.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.865+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:56.45 +02:17:18.9: 12.32 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:56.45 +02:17:18.9: 12.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 4268470165287324416,2461186.6984,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268470165287324416 20260526.1984 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 26.1984 2461186.6984 11.32 19:07:05.52 +02:58:50.8
37.37175 -2.11748 galactic Aql Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.7848+02.9863 | 19:07:05.56 +02:58:51.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-0.032 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:05.52 +02:58:50.8: 12.25 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:05.52 +02:58:50.8: 12.30 +/- 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
ATO J286.7848+02.9863,2461186.6984,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.7848+02.9863 20260526.1984 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 26.1984 2461186.6984 11.07 19:08:04.67 +01:55:53.5
36.55155 -2.81753 galactic Aql Second-epoch detections are separated by 0.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.0297+01.9266 | 19:08:04.67 +01:55:53.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.809+/-0.030 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:04.67 +01:55:53.5: 12.26 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:04.67 +01:55:53.5: 12.27 +/- 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 J287.0297+01.9266,2461186.6984,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0297+01.9266 20260526.1984 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 26.1984 2461186.6984 11.11 19:09:06.51 +02:34:27.6
37.24165 -2.75139 galactic Aql Second-epoch detections are separated by 1.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268106020775224192 | 19:09:06.35 +02:34:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:09:06.51 +02:34:27.6: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:09:06.51 +02:34:27.6: 99.00 +/- 99.00 bad_region
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 4268106020775224192,2461186.6984,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268106020775224192 20260526.1984 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.38 19:08:00.29 +02:38:46.5
37.17896 -2.47350 galactic Aql Second-epoch detections are separated by 1.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268862862738796544 | 19:08:00.30 +02:38:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.385+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:00.29 +02:38:46.5: 12.61 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:00.29 +02:38:46.5: 12.66 +/- 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
Gaia DR3 4268862862738796544,2461186.6984,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268862862738796544 20260526.1984 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 26.1984 2461186.6984 10.81 19:08:00.01 +02:18:43.4
36.88118 -2.62579 galactic Aql Second-epoch detections are separated by 1.3" and 5.3 pix
The object was found in VSX20" ZTF J190801.26+021848.8
Type: SR
# Max. Min./Amp. JD0 Period
17.767 r Y 0.625 r 2458557.08680 463.592391800000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:00.01 +02:18:43.4: 11.76 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:00.01 +02:18:43.4: 11.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.79 +/- 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 J190801.26+021848.8,2461186.6984,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190801.26+021848.8 20260526.1984 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.60 19:08:24.76 +03:07:17.8
37.64843 -2.34573 galactic Aql Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.1097+03.1318 | 19:08:24.74 +03:07:16.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +03 105 J-Ks=1.214+/-0.035 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:24.76 +03:07:17.8: 12.82 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:24.76 +03:07:17.8: 12.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 J287.1097+03.1318,2461186.6984,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1097+03.1318 20260526.1984 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 26.1984 2461186.6984 10.83 19:08:16.80 +03:16:51.9
37.77498 -2.24307 galactic Aql Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268967423782563328 | 19:08:16.89 +03:16:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1964AbaOB..31...27A [A64] Red +03 102 J-Ks=1.074+/-0.033 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:16.80 +03:16:51.9: 11.76 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:16.80 +03:16:51.9: 11.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.79 +/- 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 4268967423782563328,2461186.6984,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268967423782563328 20260526.1984 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.12 19:06:39.73 +01:54:05.3
36.36252 -2.51692 galactic Aql Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267670614176575104 | 19:06:39.74 +01:54:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.695+/-0.030 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:39.73 +01:54:05.3: 12.22 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:39.73 +01:54:05.3: 12.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 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 4267670614176575104,2461186.6984,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267670614176575104 20260526.1984 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 26.1984 2461186.6984 11.14 19:08:26.37 +02:59:04.3
37.52963 -2.41464 galactic Aql Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.1089+02.9967 | 19:08:26.33 +02:59:05.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:26.37 +02:59:04.3: 12.22 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:26.37 +02:59:04.3: 12.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 J287.1089+02.9967,2461186.6984,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1089+02.9967 20260526.1984 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 26.1984 2461186.6984 10.74 19:06:49.97 +01:49:18.0
36.31107 -2.59139 galactic Aql Second-epoch detections are separated by 0.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267668827470168192 | 19:06:49.80 +01:49:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.108+/-0.050 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:49.97 +01:49:18.0: 11.70 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:49.97 +01:49:18.0: 11.83 +/- 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
Gaia DR3 4267668827470168192,2461186.6984,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267668827470168192 20260526.1984 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 26.1984 2461186.6984 10.67 19:07:38.02 +01:53:34.9
36.46636 -2.73655 galactic Aql Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9080+01.8802 | 19:07:37.94 +01:53:34.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.240+/-0.038 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:38.02 +01:53:34.9: 11.72 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:38.02 +01:53:34.9: 11.86 +/- 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 J286.9080+01.8802,2461186.6984,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9080+01.8802 20260526.1984 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.69 19:08:59.06 +02:28:18.8
37.13628 -2.77087 galactic Aql Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268102756600082560 | 19:08:58.95 +02:28:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.520+/-0.050 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:59.06 +02:28:18.8: 11.72 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:59.06 +02:28:18.8: 99.00 +/- 99.00 bad_region
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
Gaia DR3 4268102756600082560,2461186.6984,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268102756600082560 20260526.1984 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.41 19:07:24.51 +01:52:39.5
36.42685 -2.69360 galactic Aql Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX21" ZTF J190723.47+015254.2
Type: SR
# Max. Min./Amp. JD0 Period
17.036 r Y 0.128 r 2458287.02360 39.589443100000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:24.51 +01:52:39.5: 12.55 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:24.51 +01:52:39.5: 12.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 J190723.47+015254.2,2461186.6984,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190723.47+015254.2 20260526.1984 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 26.1984 2461186.6984 11.56 19:08:23.22 +02:21:10.7
36.96195 -2.69288 galactic Aql Second-epoch detections are separated by 2.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.0959+02.3513 | 19:08:23.22 +02:21:10.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:23.22 +02:21:10.7: 12.53 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:23.22 +02:21:10.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.53 +/- 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 J287.0959+02.3513,2461186.6984,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0959+02.3513 20260526.1984 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 26.1984 2461186.6984 10.79 19:07:27.63 +02:45:54.9
37.22235 -2.29812 galactic Aql Second-epoch detections are separated by 1.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268877156389950208 | 19:07:27.62 +02:45:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.195+/-0.037 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:27.63 +02:45:54.9: 11.70 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:27.63 +02:45:54.9: 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
Gaia DR3 4268877156389950208,2461186.6984,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268877156389950208 20260526.1984 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 26.1984 2461186.6984 10.70 19:06:59.98 +01:55:17.3
36.41899 -2.58271 galactic Aql Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267693948782409344 | 19:07:00.00 +01:55:16.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1964AbaOB..31...27A [A64] Red +01 84 J-Ks=0.964+/-0.034 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:59.98 +01:55:17.3: 11.71 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:59.98 +01:55:17.3: 11.78 +/- 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
Gaia DR3 4267693948782409344,2461186.6984,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267693948782409344 20260526.1984 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 26.1984 2461186.6984 11.26 19:08:14.46 +02:45:19.1
37.30303 -2.47585 galactic Aql Second-epoch detections are separated by 1.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268865783312580352 | 19:08:14.37 +02:45:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.245+/-0.036 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:14.46 +02:45:19.1: 12.18 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:14.46 +02:45:19.1: 12.29 +/- 0.03 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
Gaia DR3 4268865783312580352,2461186.6984,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268865783312580352 20260526.1984 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 26.1984 2461186.6984 11.44 19:08:22.00 +03:12:18.8
37.71748 -2.29713 galactic Aql Second-epoch detections are separated by 2.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.0898+03.2081 | 19:08:22.01 +03:12:19.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.928+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:22.00 +03:12:18.8: 12.53 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:22.00 +03:12:18.8: 12.66 +/- 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 J287.0898+03.2081,2461186.6984,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0898+03.2081 20260526.1984 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 26.1984 2461186.6984 11.37 19:07:25.57 +01:51:19.9
36.40920 -2.70765 galactic Aql Second-epoch detections are separated by 2.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8567+01.8553 | 19:07:25.61 +01:51:19.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.235+/-0.030 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:25.57 +01:51:19.9: 12.51 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:25.57 +01:51:19.9: 12.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 J286.8567+01.8553,2461186.6984,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8567+01.8553 20260526.1984 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 26.1984 2461186.6984 10.61 19:07:31.34 +01:49:27.4
36.39242 -2.74333 galactic Aql Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8726+01.8282 | 19:07:31.35 +01:49:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.745+/-0.030 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:31.34 +01:49:27.4: 11.68 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:31.34 +01:49:27.4: 11.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.69 +/- 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 J286.8726+01.8282,2461186.6984,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8726+01.8282 20260526.1984 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.76 19:07:14.30 +02:39:18.0
37.09884 -2.29940 galactic Aql Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268869532878259712 | 19:07:14.24 +02:39:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.815+/-0.035 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:14.30 +02:39:18.0: 11.67 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:14.30 +02:39:18.0: 11.75 +/- 0.01 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 4268869532878259712,2461186.6984,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268869532878259712 20260526.1984 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 26.1984 2461186.6984 11.32 19:08:07.71 +02:09:14.4
36.75530 -2.72677 galactic Aql Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267705046977916160 | 19:08:07.78 +02:09:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.402+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:07.71 +02:09:14.4: 12.50 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:07.71 +02:09:14.4: 12.54 +/- 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
Gaia DR3 4267705046977916160,2461186.6984,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267705046977916160 20260526.1984 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 26.1984 2461186.6984 11.49 19:08:14.48 +02:37:27.0
37.18645 -2.53611 galactic Aql Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX13" Gaia DR3 4268859190597532672
Type: E
# Max. Min./Amp. JD0 Period
16.030 G 16.500 G 1.386380000000 A
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:14.48 +02:37:27.0: 12.49 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:14.48 +02:37:27.0: 12.57 +/- 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
Gaia DR3 4268859190597532672,2461186.6984,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268859190597532672 20260526.1984 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 26.1984 2461186.6984 10.66 19:07:56.31 +02:31:46.7
37.06764 -2.51229 galactic Aql Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9769+02.5300 | 19:07:56.35 +02:31:47.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.815+/-0.040 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:56.31 +02:31:46.7: 11.65 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:56.31 +02:31:46.7: 11.74 +/- 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
ATO J286.9769+02.5300,2461186.6984,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9769+02.5300 20260526.1984 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 26.1984 2461186.6984 10.65 19:07:57.26 +02:11:27.4
36.76819 -2.67116 galactic Aql Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9785+02.1950 | 19:07:57.26 +02:11:27.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.529+/-0.030 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:57.26 +02:11:27.4: 11.63 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:57.26 +02:11:27.4: 11.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.66 +/- 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 J286.9785+02.1950,2461186.6984,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9785+02.1950 20260526.1984 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.34 19:06:33.58 +01:53:54.5
36.34811 -2.49553 galactic Aql Second-epoch detections are separated by 0.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6446+01.8900 | 19:06:33.56 +01:53:54.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.808+/-0.035 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:33.58 +01:53:54.5: 12.49 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:33.58 +01:53:54.5: 12.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 J286.6446+01.8900,2461186.6984,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6446+01.8900 20260526.1984 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 26.1984 2461186.6984 11.18 19:05:25.84 +01:48:08.8
36.13336 -2.28873 galactic Aql Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267677451767695488 | 19:05:25.84 +01:48:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.602+/-0.030 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:25.84 +01:48:08.8: 12.16 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:25.84 +01:48:08.8: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 4267677451767695488,2461186.6984,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267677451767695488 20260526.1984 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 26.1984 2461186.6984 10.70 19:05:56.32 +01:51:52.1
36.24672 -2.37317 galactic Aql Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.4762+01.8578 | 19:05:56.31 +01:51:52.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.173+/-0.048 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:56.32 +01:51:52.1: 11.62 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:56.32 +01:51:52.1: 11.74 +/- 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 J286.4762+01.8578,2461186.6984,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.4762+01.8578 20260526.1984 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 26.1984 2461186.6984 11.17 19:07:03.66 +02:50:40.3
37.24705 -2.17311 galactic Aql Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.7631+02.8466 | 19:07:03.74 +02:50:39.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +02 108 J-Ks=1.202+/-0.027 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:03.66 +02:50:40.3: 12.14 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:03.66 +02:50:40.3: 12.20 +/- 0.02 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 J286.7631+02.8466,2461186.6984,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.7631+02.8466 20260526.1984 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 26.1984 2461186.6984 11.12 19:08:11.84 +02:38:41.4
37.19978 -2.51686 galactic Aql Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.0468+02.6535 | 19:08:11.77 +02:38:41.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.274+/-0.035 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:11.84 +02:38:41.4: 12.14 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:11.84 +02:38:41.4: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 J287.0468+02.6535,2461186.6984,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0468+02.6535 20260526.1984 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 26.1984 2461186.6984 10.61 19:07:07.90 +02:10:18.8
36.65691 -2.49726 galactic Aql Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.7861+02.1680 | 19:07:07.87 +02:10:18.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.157+/-0.031 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:07.90 +02:10:18.8: 11.52 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:07.90 +02:10:18.8: 11.71 +/- 0.01 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
ATO J286.7861+02.1680,2461186.6984,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.7861+02.1680 20260526.1984 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.46 19:07:43.77 +01:56:52.6
36.52621 -2.73266 galactic Aql Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267691955917264512 | 19:07:43.86 +01:56:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M5 1964AbaOB..31...27A [A64] Red +01 99 J-Ks=1.410+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:43.77 +01:56:52.6: 11.47 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:43.77 +01:56:52.6: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 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 4267691955917264512,2461186.6984,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267691955917264512 20260526.1984 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.41 19:04:55.91 +01:47:38.0
36.06865 -2.18183 galactic Aql Second-epoch detections are separated by 4.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267676524054759680 | 19:04:55.86 +01:47:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.454+/-0.033 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:04:55.91 +01:47:38.0: 12.47 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:04:55.91 +01:47:38.0: 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
Gaia DR3 4267676524054759680,2461186.6984,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267676524054759680 20260526.1984 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 26.1984 2461186.6984 11.04 19:07:39.63 +02:42:38.2
37.19670 -2.36757 galactic Aql Second-epoch detections are separated by 1.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9167+02.7215 | 19:07:39.66 +02:42:38.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M2 1964AbaOB..31...27A [A64] Red +02 119 J-Ks=1.227+/-0.039 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:39.63 +02:42:38.2: 12.10 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:39.63 +02:42:38.2: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 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
ATO J286.9167+02.7215,2461186.6984,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9167+02.7215 20260526.1984 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 26.1984 2461186.6984 10.50 19:07:54.13 +02:29:27.7
37.02913 -2.52194 galactic Aql Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9770+02.5023 | 19:07:54.10 +02:29:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.255+/-0.033 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:54.13 +02:29:27.7: 11.46 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:54.13 +02:29:27.7: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 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 J286.9770+02.5023,2461186.6984,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9770+02.5023 20260526.1984 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.50 19:05:39.20 +01:49:45.6
36.18278 -2.32588 galactic Aql Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267675050924426624 | 19:05:39.22 +01:49:45.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1964AbaOB..31...27A [A64] Red +01 70 J-Ks=1.057+/-0.028 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:39.20 +01:49:45.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:39.20 +01:49:45.6: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 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 4267675050924426624,2461186.6984,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267675050924426624 20260526.1984 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.58 19:08:44.66 +02:29:02.4
37.11950 -2.71205 galactic Aql Second-epoch detections are separated by 2.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.1780+02.4838 | 19:08:44.66 +02:29:02.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.203+/-0.075 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:44.66 +02:29:02.4: 12.76 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:44.66 +02:29:02.4: 99.00 +/- 99.00 bad_region
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
ATO J287.1780+02.4838,2461186.6984,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1780+02.4838 20260526.1984 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 26.1984 2461186.6984 10.33 19:07:42.24 +01:51:56.2
36.45003 -2.76473 galactic Aql Second-epoch detections are separated by 0.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267689172778232320 | 19:07:42.29 +01:51:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 1964AbaOB..31...27A [A64] Red +01 98 J-Ks=1.035+/-0.031 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:42.24 +01:51:56.2: 11.34 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:42.24 +01:51:56.2: 11.43 +/- 0.01 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 4267689172778232320,2461186.6984,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267689172778232320 20260526.1984 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.20 19:07:48.76 +02:05:56.0
36.67004 -2.68192 galactic Aql Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX16" ZTF J190748.43+020540.2
Type: RS
# Max. Min./Amp. JD0 Period
17.227 r Y 0.103 r 2458376.66630 4.867622600000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:48.76 +02:05:56.0: 11.19 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:48.76 +02:05:56.0: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 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
ZTF J190748.43+020540.2,2461186.6984,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190748.43+020540.2 20260526.1984 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.11 19:05:43.44 +02:13:12.4
36.53852 -2.16260 galactic Aql Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.4311+02.2200 | 19:05:43.48 +02:13:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.151+/-0.031 (F)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:05:43.44 +02:13:12.4: 12.01 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:05:43.44 +02:13:12.4: 12.12 +/- 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
ATO J286.4311+02.2200,2461186.6984,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.4311+02.2200 20260526.1984 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 10.80 19:07:47.23 +02:03:36.6
36.63267 -2.69402 galactic Aql Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9385+02.0652 | 19:07:47.28 +02:03:35.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.102+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:47.23 +02:03:36.6: 12.00 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:47.23 +02:03:36.6: 12.08 +/- 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
ATO J286.9385+02.0652,2461186.6984,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9385+02.0652 20260526.1984 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 26.1984 2461186.6984 11.48 19:08:27.62 +03:22:42.3
37.88219 -2.23834 galactic Aql Second-epoch detections are separated by 2.8" and 5.8 pix
The object was found in VSX14" ZTF J190826.91+032251.5
Type: EA
# Max. Min./Amp. JD0 Period
20.049 r Y 0.662 r 2458650.84200 0.305283400000
The object was not found in astcheck.
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:08:27.62 +03:22:42.3: 12.43 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:08:27.62 +03:22:42.3: 12.54 +/- 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
ZTF J190826.91+032251.5,2461186.6984,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190826.91+032251.5 20260526.1984 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 26.1984 2461186.6984 10.33 19:07:51.72 +02:08:04.8
36.70753 -2.67647 galactic Aql Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9657+02.1216 | 19:07:51.72 +02:08:04.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.730+/-0.026 (K)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:51.72 +02:08:04.8: 11.33 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:51.72 +02:08:04.8: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 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 J286.9657+02.1216,2461186.6984,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9657+02.1216 20260526.1984 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.62 19:06:33.27 +01:58:33.2
36.41640 -2.45892 galactic Aql Second-epoch detections are separated by 0.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6365+01.9636 | 19:06:33.34 +01:58:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.945+/-0.029 (M)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:06:33.27 +01:58:33.2: 12.99 +/- 0.03 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:06:33.27 +01:58:33.2: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J286.6365+01.9636,2461186.6984,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6365+01.9636 20260526.1984 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 26.1984 2461186.6984 10.36 19:07:21.73 +02:21:31.6
36.84958 -2.46274 galactic Aql Second-epoch detections are separated by 0.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268474017907892224 | 19:07:21.75 +02:21:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.035 (G)
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:21.73 +02:21:31.6: 11.29 +/- 0.01 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:21.73 +02:21:31.6: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.31 +/- 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 4268474017907892224,2461186.6984,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268474017907892224 20260526.1984 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1984 2461186.6984 11.43 19:07:58.92 +02:51:02.6
37.35817 -2.37459 galactic Aql Second-epoch detections are separated by 2.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4268879119246683776 | 19:07:58.98 +02:51:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits at 19:07:58.92 +02:51:02.6: 12.45 +/- 0.02 detection
Forced photometry on wcs_Ser-04-Q2b1x1_2026-04-16_02-29-19_20.00sec_-4.90C_LIGHTs_0233.fits at 19:07:58.92 +02:51:02.6: 12.56 +/- 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
Gaia DR3 4268879119246683776,2461186.6984,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4268879119246683776 20260526.1984 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q2b1x1_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-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Last image: 2461186.69861975 26.05.2026 04:45:50.746 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q2b1x1_234857_TTUQ2b1x1_2017996_3sLqWVBV/fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
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): 10967
Objects passed selection criteria: 10910
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 7031.25
Average stars matched: 6886 (97.9342 %)
Memory usage VmPeak: 119012 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 23:51:09 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-Q2b1x1_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-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits
Last image: 2461186.69861975 26.05.2026 04:45:50.746 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-04-Q2b1x1_234857_TTUQ2b1x1_2017996_3sLqWVBV/fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 319
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 18 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): 91474
Objects passed selection criteria: 91184
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 60674
Average stars matched: 58914 (97.0993 %)
Memory usage VmPeak: 1942780 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 23:54:03 CDT 2026
Host name: tau
############################################################
**** FOUND 18:56:14.70 +04:12:08.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173260_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 173260_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15359_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15359_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18036_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 18036_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10967_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10967_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13127_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13127_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21150_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 21150_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:47.87 +02:50:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.671 4268889869489904000 287.19939315870 +02.84088093323 12.0595 11.1640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21364_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 21364_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:00.72 +02:51:35.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15601_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 15601_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:58.05 +02:22:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11901_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11901_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:31.95 +02:01:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 1.638 4267699480699742592 287.13357014726 +02.03190435910 12.0139 11.0215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11603_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11603_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15201_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15201_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10875_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10875_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13521_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13521_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17670_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 17670_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14115_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14115_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12063_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12063_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12149_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12149_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14481_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14481_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14072_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 14072_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21281_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 21281_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:08.46 +02:51:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.984 4268888426380892288 287.28497674698 +02.85009835715 12.2800 11.3815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19170_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 19170_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28111_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 28111_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:06.93 +03:21:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 1.104 4269061358940639104 287.27916415451 +03.35218710535 12.0817 11.0891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11536_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11536_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10964_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 10964_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:00.60 +01:56:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.342 4267648039822457472 287.25223378826 +01.93921128729 12.1104 11.2566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22669_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 22669_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14202_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14202_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19623_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 19623_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15794_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 15794_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:18.65 +02:24:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 2.607 4268096816720877056 287.07825801291 +02.40319468325 11.0264 9.6263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18370_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 18370_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11880_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11880_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:26.03 +02:02:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 3.913 4267698209390784256 287.10864095155 +02.03353965885 11.0942 9.5845 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12924_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12924_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17182_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 17182_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:59.65 +02:30:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 1.512 4268103718672755200 287.24813800180 +02.50522857122 12.6632 11.7492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10802_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10802_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15226_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15226_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18979_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 18979_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:06:33.37 +02:41:48.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19923_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 19923_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24328_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 24328_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12344_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12344_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18334_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 18334_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:49.57 +02:36:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 0.984 4268109770315917824 287.20657520036 +02.61382674707 11.8824 10.8159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13948_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 13948_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:45.89 +02:13:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.550 4268080422770156544 287.19135951946 +02.22613429814 12.2309 11.7150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24244_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 24244_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:07.71 +03:04:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 1.377 4268912070238214016 287.28241863251 +03.07093995474 12.0089 11.1042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16452_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 16452_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15891_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15891_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15504_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 15504_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:44.37 +02:22:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 0.294 4268095884652413184 287.18479372642 +02.37271475082 10.8293 10.0021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21903_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 21903_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29603_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 29603_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:11.53 +03:27:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.685 4269064730567128832 287.29814666758 +03.46336898063 11.5003 10.5576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167269_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 167269_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 18:29:55.86 +09:50:21.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32255_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 32255_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:07.97 +03:39:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 0.143 4269087751593762432 287.28322501931 +03.65925815360 11.5534 10.6763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09981_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 09981_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:32.38 +01:51:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.19, MAG_FAINT_SEARCH_LIMIT=11.17)GAIADR2_OUTPUT=# 0.056 4267640003989716736 287.13490191627 +01.85122760397 11.0216 10.6196 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12091_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12091_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17517_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 17517_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11441_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11441_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18461_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 18461_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20482_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 20482_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09693_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 09693_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:36.38 +01:49:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.13, MAG_FAINT_SEARCH_LIMIT=11.11)GAIADR2_OUTPUT=# 0.901 4267639694752638080 287.15179973813 +01.82304073846 10.6159 9.7032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11918_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11918_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10776_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 10776_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:12.29 +01:55:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.228 4267644294610976256 287.05101937086 +01.91858956435 12.2915 11.8944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23309_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 23309_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18634_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 18634_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:45.92 +02:38:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.060 4268110040864611840 287.19155902186 +02.64105061801 12.2370 11.3294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15296_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15296_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17407_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 17407_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11835_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11835_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19488_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 19488_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:47.62 +02:42:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 2.619 4268861488346014336 287.19783189131 +02.70948915479 12.3734 11.6265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18333_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 18333_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:02.37 +02:36:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 2.008 4268109284950368384 287.25933585282 +02.61308968345 12.3393 11.6416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32493_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 32493_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:14.59 +03:40:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 1.060 4269089194703173504 287.31051516941 +03.67239761083 11.8051 11.3797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11971_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11971_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26720_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 26720_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23822_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 23822_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13806_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13806_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10976_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10976_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10982_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10982_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14679_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14679_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27275_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 27275_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10312_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10312_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28659_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 28659_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:49.41 +03:23:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.382 4269062531543877504 287.20562122073 +03.39482270033 12.2142 11.6796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28192_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 28192_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:00.16 +03:21:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 1.107 4269061530739327744 287.25083444083 +03.36388113227 11.8667 10.9578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09287_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09287_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20061_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 20061_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:08.56 +02:45:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 0.693 4268885441439900160 287.28554496075 +02.75953801618 11.6523 11.0559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21803_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 21803_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15400_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15400_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11669_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11669_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09773_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09773_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09936_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09936_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20270_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 20270_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10131_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10131_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13190_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 13190_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:28.28 +02:09:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 1.121 4267704492872590208 287.11810568452 +02.15887651720 11.2869 10.2819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09851_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09851_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12591_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 12591_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:52.90 +02:05:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 0.954 4267700129185818368 287.22058154793 +02.08926483154 11.7928 10.8136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12292_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12292_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09607_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 09607_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:52.69 +01:48:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 1.128 4267644505115092992 287.21923469662 +01.80653523837 11.6732 11.2227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20427_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 20427_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10854_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10854_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14359_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14359_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14585_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 14585_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:22.04 +02:17:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.353 4268093582549948800 287.09119325766 +02.28319841096 12.3851 11.7840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127739_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 127739_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 18:31:02.73 +09:40:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14939_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14939_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32270_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 32270_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:55.30 +03:41:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 0.626 4269088846731284736 287.23025496292 +03.69348164701 12.3381 11.6396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15743_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 15743_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:25.10 +02:25:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 0.836 4268097229037731840 287.10478194842 +02.41849073126 11.0709 9.9532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12827_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12827_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14635_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 14635_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:18.77 +02:17:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 1.126 4268093273312303104 287.07792079465 +02.28740406180 12.4294 11.7100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10347_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10347_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11618_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11618_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:46.86 +02:00:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 0.816 4267652162991059072 287.19503195358 +02.00063211668 11.6334 11.2201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19136_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 19136_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:48.55 +02:41:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 0.840 4268861286542258688 287.20205919018 +02.68941018612 11.3734 10.5077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14532_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14532_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22818_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 22818_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10795_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10795_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17902_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 17902_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18677_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 18677_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16761_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 16761_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:33.35 +02:30:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.71, MAG_FAINT_SEARCH_LIMIT=10.69)GAIADR2_OUTPUT=# 0.919 4268106643606105600 287.13920566552 +02.50235268005 9.5168 8.2154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14809_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 14809_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24888_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 24888_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26898_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 26898_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10489_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10489_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13197_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 13197_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:51.57 +02:08:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.476 4268075921644434432 287.21524026811 +02.14584076324 12.0246 10.8424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22986_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 22986_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20635_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 20635_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:11.22 +02:48:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.209 4268887189430312576 287.29664405524 +02.80159650652 12.3488 11.7466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17844_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 17844_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:09.76 +02:34:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 1.317 4268105956411904256 287.29032586184 +02.57213358455 11.2629 10.2643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09709_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09709_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11010_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11010_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:40.39 +01:56:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10428_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10428_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16656_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 16656_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10352_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10352_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15314_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15314_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20062_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 20062_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10723_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10723_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19990_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 19990_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13291_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 13291_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:29.94 +02:10:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 0.239 4267704531581685888 287.12473198220 +02.16871396443 11.4037 10.6870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11155_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11155_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:11.06 +01:57:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 0.609 4267697277327537664 287.04594013782 +01.96177096342 11.5336 10.9841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25984_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 25984_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12568_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 12568_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28822_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 28822_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:39.53 +03:25:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 0.967 4269065830078837760 287.16485824961 +03.41938973888 11.0133 9.9004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10083_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10083_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09708_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09708_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18701_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 18701_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13207_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13207_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18435_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 18435_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20924_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 20924_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:34.79 +02:49:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.120 4268889594611997440 287.14495327693 +02.82817177474 12.3699 11.9560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17214_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 17214_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29667_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 29667_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:38.64 +03:27:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 0.797 4269066787779280640 287.16088377316 +03.46204974571 12.1327 11.3285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13502_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13502_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10452_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10452_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09495_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09495_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11528_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11528_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:23.14 +01:59:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 1.045 4267697861443088640 287.09642220130 +01.99873752918 11.2453 10.3932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15539_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 15539_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:59.92 +02:22:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10082_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10082_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09786_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 09786_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:45.55 +01:50:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 0.680 4267644779993164032 287.18998000851 +01.83337655257 12.1813 11.4912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25482_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 25482_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:09.55 +03:09:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 0.387 4268915196974667904 287.28980895504 +03.16318942416 11.9168 11.2915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21128_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 21128_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18469_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 18469_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16310_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 16310_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:43.48 +02:25:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.989 4268102928398775936 287.18096592060 +02.43052093147 12.4523 11.2736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13333_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13333_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13585_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 13585_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:07.35 +02:11:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.494 4268076437040508032 287.28076177790 +02.19043369280 11.7596 10.8806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10886_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 10886_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09379_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09379_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19409_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 19409_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17788_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 17788_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:01.25 +02:34:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 1.474 4268108597755601920 287.25486819268 +02.57336730568 11.7854 10.9179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16895_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 16895_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09670_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09670_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25323_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 25323_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:58.20 +03:09:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 0.133 4268917705235644928 287.24253659017 +03.15624544016 11.2809 10.7750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22625_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 22625_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:06.31 +02:57:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.583 4268898979177529344 287.27644801475 +02.95376496996 11.6262 10.6940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16875_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 16875_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19214_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 19214_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:59.99 +02:41:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 2.097 4268134023967775744 287.24938335869 +02.68681994394 12.3331 11.4380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14329_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 14329_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:56.33 +02:15:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 3.002 4268082072037597056 287.23522188596 +02.25131491433 12.5484 11.5612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16897_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 16897_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:50.66 +02:29:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 1.001 4268103546874064384 287.21084745338 +02.48414738689 11.8216 11.2681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09916_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 09916_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09659_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 09659_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:19.01 +01:48:58.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.40, MAG_FAINT_SEARCH_LIMIT=11.38)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12150_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12150_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29770_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 29770_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:41.81 +03:28:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 0.204 4269068299641590400 287.17420147137 +03.47850074027 11.6155 10.7211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19684_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 19684_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:07.11 +02:43:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.430 4268134608083326208 287.27923016915 +02.72428531525 12.2955 11.7542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13826_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 13826_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25480_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 25480_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:46.92 +03:10:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 0.239 4268918014473431680 287.19555876317 +03.17930888990 10.8977 9.9946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12208_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12208_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14701_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 14701_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:26.91 +02:17:36.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28397_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 28397_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17697_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 17697_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:31.30 +02:33:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.339 4268107983635982464 287.13034354330 +02.56614253704 12.0933 11.1427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22837_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 22837_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:58.02 +02:58:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 0.810 4268899318414459648 287.24191767613 +02.98018287825 12.1779 11.3042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12923_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 12923_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11341_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 11341_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15312_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 15312_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11076_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 11076_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:08:30.83 +01:57:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 1.546 4267650552429731072 287.12868179893 +01.95660550576 10.7603 9.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13170_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 13170_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 19:09:01.88 +02:09:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.553 4268076059083387520 287.25793732078 +02.15147005037 11.9536 10.9825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21126_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
Preparing report for the candidate 21126_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10408_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127
The candidate 10408_fd_Ser-04-Q2b1x1_2026-05-25_23-45-50_20.00sec_5.00C_LIGHT_0127 did not pass the final checks
**** FOUND 18:44:49.99 +02:03:37.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 237s
Prepared the HTML report for the field Ser-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:07:42.37 +01:47:57.2
19:04:55.91 +01:47:38.0
19:05:25.84 +01:48:08.8
19:05:39.20 +01:49:45.6
19:07:31.34 +01:49:27.4
19:06:49.97 +01:49:18.0
19:06:42.55 +01:50:48.7
19:07:32.71 +01:50:08.0
19:07:42.24 +01:51:56.2
19:05:20.75 +01:50:52.0
19:05:56.32 +01:51:52.1
19:07:25.57 +01:51:19.9
19:05:20.25 +01:52:13.2
19:05:50.36 +01:52:58.5
19:06:48.29 +01:53:15.3
19:07:24.51 +01:52:39.5
19:07:38.02 +01:53:34.9
19:06:33.58 +01:53:54.5
19:06:39.73 +01:54:05.3
19:06:59.98 +01:55:17.3
19:08:04.67 +01:55:53.5
19:07:52.14 +01:55:20.3
19:05:51.10 +01:56:43.4
19:05:59.00 +01:56:09.7
19:07:43.77 +01:56:52.6
19:06:23.35 +01:56:28.2
19:07:55.27 +02:02:15.1
19:07:48.23 +01:56:29.2
19:06:33.27 +01:58:33.2
19:07:45.47 +01:59:16.1
19:06:25.40 +01:59:40.2
18:43:36.35 +02:04:16.7
19:07:48.68 +02:01:05.7
19:07:20.69 +02:02:18.1
19:05:44.82 +02:02:31.9
19:07:47.68 +02:02:07.7
19:06:40.69 +02:02:59.1
19:07:38.10 +02:03:28.3
19:06:10.29 +02:03:04.0
19:07:48.76 +02:05:56.0
19:07:47.23 +02:03:36.6
19:06:46.38 +02:04:19.6
19:08:11.46 +02:05:51.0
18:42:50.40 +02:11:29.7
19:07:51.72 +02:08:04.8
19:07:19.21 +02:08:06.2
19:06:47.96 +02:08:43.7
19:08:07.71 +02:09:14.4
19:07:07.90 +02:10:18.8
19:07:57.26 +02:11:27.4
19:07:39.68 +02:11:07.2
19:07:32.99 +02:13:42.1
19:05:43.44 +02:13:12.4
19:07:26.74 +02:14:39.4
19:07:20.99 +02:15:05.5
19:06:46.37 +02:16:28.1
19:08:05.19 +02:16:24.4
19:05:56.45 +02:17:18.9
19:06:21.96 +02:18:10.7
19:08:00.01 +02:18:43.4
19:08:31.82 +02:19:12.8
19:08:59.41 +02:20:11.8
19:08:02.39 +02:20:34.3
19:06:42.67 +02:20:52.3
19:07:21.73 +02:21:31.6
19:08:23.22 +02:21:10.7
19:08:12.89 +02:21:06.3
19:07:09.43 +02:21:50.5
19:06:39.57 +02:24:16.7
19:06:43.12 +02:28:57.5
19:08:59.06 +02:28:18.8
19:08:44.66 +02:29:02.4
19:07:54.13 +02:29:27.7
19:07:56.31 +02:31:46.7
19:07:38.79 +02:32:39.1
19:08:13.69 +02:33:15.2
19:07:25.90 +02:35:57.3
19:09:06.51 +02:34:27.6
19:07:22.39 +02:37:13.5
19:08:14.48 +02:37:27.0
19:07:11.28 +02:37:34.2
19:08:11.84 +02:38:41.4
19:08:00.29 +02:38:46.5
19:07:14.30 +02:39:18.0
19:08:45.19 +02:40:45.7
19:07:39.63 +02:42:38.2
19:07:53.71 +02:43:38.3
19:08:11.23 +02:44:50.7
19:08:14.46 +02:45:19.1
19:07:27.63 +02:45:54.9
19:08:33.03 +02:46:56.7
19:07:40.86 +02:47:19.4
19:07:31.91 +02:47:51.9
19:07:58.92 +02:51:02.6
19:07:03.66 +02:50:40.3
19:08:24.18 +02:53:37.2
19:07:05.52 +02:58:50.8
19:08:26.37 +02:59:04.3
19:07:38.28 +03:00:46.9
19:08:04.13 +03:04:09.4
19:08:01.58 +03:04:56.0
19:08:24.76 +03:07:17.8
19:08:22.00 +03:12:18.8
19:07:59.70 +03:16:25.6
19:08:16.80 +03:16:51.9
19:08:27.62 +03:22:42.3
########### Completed Ser-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:08:12.89 +02:21:06.3
19:07:22.39 +02:37:13.5
19:06:23.35 +01:56:28.2
19:06:47.96 +02:08:43.7
18:43:36.35 +02:04:16.7
19:08:59.41 +02:20:11.8
19:05:59.00 +01:56:09.7
19:07:39.68 +02:11:07.2
19:07:25.90 +02:35:57.3
19:07:26.74 +02:14:39.4
19:06:40.69 +02:02:59.1
19:06:10.29 +02:03:04.0
19:08:05.19 +02:16:24.4
19:08:45.19 +02:40:45.7
19:06:25.40 +01:59:40.2
19:07:20.99 +02:15:05.5
19:07:53.71 +02:43:38.3
19:07:19.21 +02:08:06.2
19:07:52.14 +01:55:20.3
19:08:02.39 +02:20:34.3
19:08:11.23 +02:44:50.7
19:08:01.58 +03:04:56.0
19:08:11.46 +02:05:51.0
19:06:43.12 +02:28:57.5
19:06:39.57 +02:24:16.7
19:07:38.10 +02:03:28.3
19:08:13.69 +02:33:15.2
19:07:45.47 +01:59:16.1
19:07:11.28 +02:37:34.2
19:07:31.91 +02:47:51.9
19:05:44.82 +02:02:31.9
19:07:38.28 +03:00:46.9
19:06:42.67 +02:20:52.3
19:07:38.79 +02:32:39.1
19:07:20.69 +02:02:18.1
19:07:47.68 +02:02:07.7
19:07:59.70 +03:16:25.6
19:08:04.13 +03:04:09.4
19:07:32.99 +02:13:42.1
19:07:55.27 +02:02:15.1
19:07:48.23 +01:56:29.2
19:06:21.96 +02:18:10.7
19:05:50.36 +01:52:58.5
19:07:42.37 +01:47:57.2
19:08:24.18 +02:53:37.2
19:07:09.43 +02:21:50.5
19:07:48.68 +02:01:05.7
19:06:42.55 +01:50:48.7
19:05:20.75 +01:50:52.0
19:08:33.03 +02:46:56.7
19:05:20.25 +01:52:13.2
19:07:32.71 +01:50:08.0
19:06:46.38 +02:04:19.6
19:07:40.86 +02:47:19.4
19:05:51.10 +01:56:43.4
19:06:46.37 +02:16:28.1
19:08:31.82 +02:19:12.8
18:42:50.40 +02:11:29.7
19:06:48.29 +01:53:15.3
19:05:56.45 +02:17:18.9
19:07:05.52 +02:58:50.8
19:08:04.67 +01:55:53.5
19:09:06.51 +02:34:27.6
19:08:00.29 +02:38:46.5
19:08:00.01 +02:18:43.4
19:08:24.76 +03:07:17.8
19:08:16.80 +03:16:51.9
19:06:39.73 +01:54:05.3
19:08:26.37 +02:59:04.3
19:06:49.97 +01:49:18.0
19:07:38.02 +01:53:34.9
19:08:59.06 +02:28:18.8
19:07:24.51 +01:52:39.5
19:08:23.22 +02:21:10.7
19:07:27.63 +02:45:54.9
19:06:59.98 +01:55:17.3
19:08:14.46 +02:45:19.1
19:08:22.00 +03:12:18.8
19:07:25.57 +01:51:19.9
19:07:31.34 +01:49:27.4
19:07:14.30 +02:39:18.0
19:08:07.71 +02:09:14.4
19:08:14.48 +02:37:27.0
19:07:56.31 +02:31:46.7
19:07:57.26 +02:11:27.4
19:06:33.58 +01:53:54.5
19:05:25.84 +01:48:08.8
19:05:56.32 +01:51:52.1
19:07:03.66 +02:50:40.3
19:08:11.84 +02:38:41.4
19:07:07.90 +02:10:18.8
19:07:43.77 +01:56:52.6
19:04:55.91 +01:47:38.0
19:07:39.63 +02:42:38.2
19:07:54.13 +02:29:27.7
19:05:39.20 +01:49:45.6
19:08:44.66 +02:29:02.4
19:07:42.24 +01:51:56.2
19:07:48.76 +02:05:56.0
19:05:43.44 +02:13:12.4
19:07:47.23 +02:03:36.6
19:08:27.62 +03:22:42.3
19:07:51.72 +02:08:04.8
19:06:33.27 +01:58:33.2
19:07:21.73 +02:21:31.6
19:07:58.92 +02:51:02.6
###################################################################################
19:08:12.89 +02:21:06.3 -- not an asteroid (will add it to exclusion list)
19:07:22.39 +02:37:13.5 -- not an asteroid (will add it to exclusion list)
19:06:23.35 +01:56:28.2 -- not an asteroid (will add it to exclusion list)
19:06:47.96 +02:08:43.7 -- not an asteroid (will add it to exclusion list)
18:43:36.35 +02:04:16.7 -- not an asteroid (will add it to exclusion list)
19:08:59.41 +02:20:11.8 -- not an asteroid (will add it to exclusion list)
19:05:59.00 +01:56:09.7 -- not an asteroid (will add it to exclusion list)
19:07:39.68 +02:11:07.2 -- not an asteroid (will add it to exclusion list)
19:07:25.90 +02:35:57.3 -- not an asteroid (will add it to exclusion list)
19:07:26.74 +02:14:39.4 -- not an asteroid (will add it to exclusion list)
19:06:40.69 +02:02:59.1 -- not an asteroid (will add it to exclusion list)
19:06:10.29 +02:03:04.0 -- not an asteroid (will add it to exclusion list)
19:08:05.19 +02:16:24.4 -- not an asteroid (will add it to exclusion list)
19:08:45.19 +02:40:45.7 -- not an asteroid (will add it to exclusion list)
19:06:25.40 +01:59:40.2 -- not an asteroid (will add it to exclusion list)
19:07:20.99 +02:15:05.5 -- not an asteroid (will add it to exclusion list)
19:07:53.71 +02:43:38.3 -- not an asteroid (will add it to exclusion list)
19:07:19.21 +02:08:06.2 -- not an asteroid (will add it to exclusion list)
19:07:52.14 +01:55:20.3 -- not an asteroid (will add it to exclusion list)
19:08:02.39 +02:20:34.3 -- not an asteroid (will add it to exclusion list)
19:08:11.23 +02:44:50.7 -- not an asteroid (will add it to exclusion list)
19:08:01.58 +03:04:56.0 -- not an asteroid (will add it to exclusion list)
19:08:11.46 +02:05:51.0 -- not an asteroid (will add it to exclusion list)
19:06:43.12 +02:28:57.5 -- not an asteroid (will add it to exclusion list)
19:06:39.57 +02:24:16.7 -- not an asteroid (will add it to exclusion list)
19:07:38.10 +02:03:28.3 -- not an asteroid (will add it to exclusion list)
19:08:13.69 +02:33:15.2 -- not an asteroid (will add it to exclusion list)
19:07:45.47 +01:59:16.1 -- not an asteroid (will add it to exclusion list)
19:07:11.28 +02:37:34.2 -- not an asteroid (will add it to exclusion list)
19:07:31.91 +02:47:51.9 -- not an asteroid (will add it to exclusion list)
19:05:44.82 +02:02:31.9 -- not an asteroid (will add it to exclusion list)
19:07:38.28 +03:00:46.9 -- not an asteroid (will add it to exclusion list)
19:06:42.67 +02:20:52.3 -- not an asteroid (will add it to exclusion list)
19:07:38.79 +02:32:39.1 -- not an asteroid (will add it to exclusion list)
19:07:20.69 +02:02:18.1 -- not an asteroid (will add it to exclusion list)
19:07:47.68 +02:02:07.7 -- not an asteroid (will add it to exclusion list)
19:07:59.70 +03:16:25.6 -- not an asteroid (will add it to exclusion list)
19:08:04.13 +03:04:09.4 -- not an asteroid (will add it to exclusion list)
19:07:32.99 +02:13:42.1 -- not an asteroid (will add it to exclusion list)
19:07:55.27 +02:02:15.1 -- not an asteroid (will add it to exclusion list)
19:07:48.23 +01:56:29.2 -- not an asteroid (will add it to exclusion list)
19:06:21.96 +02:18:10.7 -- not an asteroid (will add it to exclusion list)
19:05:50.36 +01:52:58.5 -- not an asteroid (will add it to exclusion list)
19:07:42.37 +01:47:57.2 -- not an asteroid (will add it to exclusion list)
19:08:24.18 +02:53:37.2 -- not an asteroid (will add it to exclusion list)
19:07:09.43 +02:21:50.5 -- not an asteroid (will add it to exclusion list)
19:07:48.68 +02:01:05.7 -- not an asteroid (will add it to exclusion list)
19:06:42.55 +01:50:48.7 -- not an asteroid (will add it to exclusion list)
19:05:20.75 +01:50:52.0 -- not an asteroid (will add it to exclusion list)
19:08:33.03 +02:46:56.7 -- not an asteroid (will add it to exclusion list)
19:05:20.25 +01:52:13.2 -- not an asteroid (will add it to exclusion list)
19:07:32.71 +01:50:08.0 -- not an asteroid (will add it to exclusion list)
19:06:46.38 +02:04:19.6 -- not an asteroid (will add it to exclusion list)
19:07:40.86 +02:47:19.4 -- not an asteroid (will add it to exclusion list)
19:05:51.10 +01:56:43.4 -- not an asteroid (will add it to exclusion list)
19:06:46.37 +02:16:28.1 -- not an asteroid (will add it to exclusion list)
19:08:31.82 +02:19:12.8 -- not an asteroid (will add it to exclusion list)
18:42:50.40 +02:11:29.7 -- not an asteroid (will add it to exclusion list)
19:06:48.29 +01:53:15.3 -- not an asteroid (will add it to exclusion list)
19:05:56.45 +02:17:18.9 -- not an asteroid (will add it to exclusion list)
19:07:05.52 +02:58:50.8 -- not an asteroid (will add it to exclusion list)
19:08:04.67 +01:55:53.5 -- not an asteroid (will add it to exclusion list)
19:09:06.51 +02:34:27.6 -- not an asteroid (will add it to exclusion list)
19:08:00.29 +02:38:46.5 -- not an asteroid (will add it to exclusion list)
19:08:00.01 +02:18:43.4 -- not an asteroid (will add it to exclusion list)
19:08:24.76 +03:07:17.8 -- not an asteroid (will add it to exclusion list)
19:08:16.80 +03:16:51.9 -- not an asteroid (will add it to exclusion list)
19:06:39.73 +01:54:05.3 -- not an asteroid (will add it to exclusion list)
19:08:26.37 +02:59:04.3 -- not an asteroid (will add it to exclusion list)
19:06:49.97 +01:49:18.0 -- not an asteroid (will add it to exclusion list)
19:07:38.02 +01:53:34.9 -- not an asteroid (will add it to exclusion list)
19:08:59.06 +02:28:18.8 -- not an asteroid (will add it to exclusion list)
19:07:24.51 +01:52:39.5 -- not an asteroid (will add it to exclusion list)
19:08:23.22 +02:21:10.7 -- not an asteroid (will add it to exclusion list)
19:07:27.63 +02:45:54.9 -- not an asteroid (will add it to exclusion list)
19:06:59.98 +01:55:17.3 -- not an asteroid (will add it to exclusion list)
19:08:14.46 +02:45:19.1 -- not an asteroid (will add it to exclusion list)
19:08:22.00 +03:12:18.8 -- not an asteroid (will add it to exclusion list)
19:07:25.57 +01:51:19.9 -- not an asteroid (will add it to exclusion list)
19:07:31.34 +01:49:27.4 -- not an asteroid (will add it to exclusion list)
19:07:14.30 +02:39:18.0 -- not an asteroid (will add it to exclusion list)
19:08:07.71 +02:09:14.4 -- not an asteroid (will add it to exclusion list)
19:08:14.48 +02:37:27.0 -- not an asteroid (will add it to exclusion list)
19:07:56.31 +02:31:46.7 -- not an asteroid (will add it to exclusion list)
19:07:57.26 +02:11:27.4 -- not an asteroid (will add it to exclusion list)
19:06:33.58 +01:53:54.5 -- not an asteroid (will add it to exclusion list)
19:05:25.84 +01:48:08.8 -- not an asteroid (will add it to exclusion list)
19:05:56.32 +01:51:52.1 -- not an asteroid (will add it to exclusion list)
19:07:03.66 +02:50:40.3 -- not an asteroid (will add it to exclusion list)
19:08:11.84 +02:38:41.4 -- not an asteroid (will add it to exclusion list)
19:07:07.90 +02:10:18.8 -- not an asteroid (will add it to exclusion list)
19:07:43.77 +01:56:52.6 -- not an asteroid (will add it to exclusion list)
19:04:55.91 +01:47:38.0 -- not an asteroid (will add it to exclusion list)
19:07:39.63 +02:42:38.2 -- not an asteroid (will add it to exclusion list)
19:07:54.13 +02:29:27.7 -- not an asteroid (will add it to exclusion list)
19:05:39.20 +01:49:45.6 -- not an asteroid (will add it to exclusion list)
19:08:44.66 +02:29:02.4 -- not an asteroid (will add it to exclusion list)
19:07:42.24 +01:51:56.2 -- not an asteroid (will add it to exclusion list)
19:07:48.76 +02:05:56.0 -- not an asteroid (will add it to exclusion list)
19:05:43.44 +02:13:12.4 -- not an asteroid (will add it to exclusion list)
19:07:47.23 +02:03:36.6 -- not an asteroid (will add it to exclusion list)
19:08:27.62 +03:22:42.3 -- not an asteroid (will add it to exclusion list)
19:07:51.72 +02:08:04.8 -- not an asteroid (will add it to exclusion list)
19:06:33.27 +01:58:33.2 -- not an asteroid (will add it to exclusion list)
19:07:21.73 +02:21:31.6 -- not an asteroid (will add it to exclusion list)
19:07:58.92 +02:51:02.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:42:50.40 +02:11:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:43:36.35 +02:04:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:55.91 +01:47:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:20.25 +01:52:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:20.75 +01:50:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:25.84 +01:48:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:39.20 +01:49:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:43.44 +02:13:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:44.82 +02:02:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:50.36 +01:52:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:51.10 +01:56:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:56.32 +01:51:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:56.45 +02:17:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:59.00 +01:56:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:10.29 +02:03:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:21.96 +02:18:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:23.35 +01:56:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:25.40 +01:59:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:33.27 +01:58:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:33.58 +01:53:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:39.57 +02:24:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:39.73 +01:54:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:40.69 +02:02:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:42.55 +01:50:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:42.67 +02:20:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:43.12 +02:28:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:46.37 +02:16:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:46.38 +02:04:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:47.96 +02:08:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:48.29 +01:53:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:49.97 +01:49:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:59.98 +01:55:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:03.66 +02:50:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:05.52 +02:58:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:07.90 +02:10:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:09.43 +02:21:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:11.28 +02:37:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:14.30 +02:39:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:19.21 +02:08:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:20.69 +02:02:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:20.99 +02:15:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:21.73 +02:21:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:22.39 +02:37:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:24.51 +01:52:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:25.57 +01:51:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:25.90 +02:35:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:26.74 +02:14:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:27.63 +02:45:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:31.34 +01:49:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:31.91 +02:47:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:32.71 +01:50:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:32.99 +02:13:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:38.02 +01:53:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:38.10 +02:03:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:38.28 +03:00:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:38.79 +02:32:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:39.63 +02:42:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:39.68 +02:11:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:40.86 +02:47:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:42.24 +01:51:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:42.37 +01:47:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:43.77 +01:56:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:45.47 +01:59:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:47.23 +02:03:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:47.68 +02:02:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:48.23 +01:56:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:48.68 +02:01:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:48.76 +02:05:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:51.72 +02:08:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:52.14 +01:55:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:53.71 +02:43:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:54.13 +02:29:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:55.27 +02:02:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:56.31 +02:31:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:57.26 +02:11:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:58.92 +02:51:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:59.70 +03:16:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:00.01 +02:18:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:00.29 +02:38:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:01.58 +03:04:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:02.39 +02:20:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:04.13 +03:04:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:04.67 +01:55:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:05.19 +02:16:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:07.71 +02:09:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:11.23 +02:44:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:11.46 +02:05:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:11.84 +02:38:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:12.89 +02:21:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:13.69 +02:33:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:14.46 +02:45:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:14.48 +02:37:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:16.80 +03:16:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:22.00 +03:12:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:23.22 +02:21:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:24.18 +02:53:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:24.76 +03:07:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:26.37 +02:59:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:27.62 +03:22:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:31.82 +02:19:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:33.03 +02:46:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:44.66 +02:29:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:45.19 +02:40:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:59.06 +02:28:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:59.41 +02:20:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:06.51 +02:34:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
18:42:50.40 +02:11:29.7 -- not a known variable star
18:43:36.35 +02:04:16.7 -- not a known variable star
19:04:55.91 +01:47:38.0 -- not a known variable star
19:05:20.25 +01:52:13.2 -- not a known variable star
19:05:20.75 +01:50:52.0 -- a known variable star
19:05:25.84 +01:48:08.8 -- not a known variable star
19:05:39.20 +01:49:45.6 -- not a known variable star
19:05:43.44 +02:13:12.4 -- not a known variable star
19:05:44.82 +02:02:31.9 -- not a known variable star
19:05:50.36 +01:52:58.5 -- not a known variable star
19:05:51.10 +01:56:43.4 -- not a known variable star
19:05:56.32 +01:51:52.1 -- not a known variable star
19:05:56.45 +02:17:18.9 -- not a known variable star
19:05:59.00 +01:56:09.7 -- not a known variable star
19:06:10.29 +02:03:04.0 -- not a known variable star
19:06:21.96 +02:18:10.7 -- not a known variable star
19:06:23.35 +01:56:28.2 -- not a known variable star
19:06:25.40 +01:59:40.2 -- not a known variable star
19:06:33.27 +01:58:33.2 -- not a known variable star
19:06:33.58 +01:53:54.5 -- not a known variable star
19:06:39.57 +02:24:16.7 -- a known variable star
19:06:39.73 +01:54:05.3 -- not a known variable star
19:06:40.69 +02:02:59.1 -- not a known variable star
19:06:42.55 +01:50:48.7 -- not a known variable star
19:06:42.67 +02:20:52.3 -- not a known variable star
19:06:43.12 +02:28:57.5 -- not a known variable star
19:06:46.37 +02:16:28.1 -- not a known variable star
19:06:46.38 +02:04:19.6 -- not a known variable star
19:06:47.96 +02:08:43.7 -- not a known variable star
19:06:48.29 +01:53:15.3 -- a known variable star
19:06:49.97 +01:49:18.0 -- not a known variable star
19:06:59.98 +01:55:17.3 -- not a known variable star
19:07:03.66 +02:50:40.3 -- not a known variable star
19:07:05.52 +02:58:50.8 -- not a known variable star
19:07:07.90 +02:10:18.8 -- not a known variable star
19:07:09.43 +02:21:50.5 -- not a known variable star
19:07:11.28 +02:37:34.2 -- not a known variable star
19:07:14.30 +02:39:18.0 -- not a known variable star
19:07:19.21 +02:08:06.2 -- not a known variable star
19:07:20.69 +02:02:18.1 -- a known variable star
19:07:20.99 +02:15:05.5 -- not a known variable star
19:07:21.73 +02:21:31.6 -- not a known variable star
19:07:22.39 +02:37:13.5 -- not a known variable star
19:07:24.51 +01:52:39.5 -- a known variable star
19:07:25.57 +01:51:19.9 -- not a known variable star
19:07:25.90 +02:35:57.3 -- not a known variable star
19:07:26.74 +02:14:39.4 -- not a known variable star
19:07:27.63 +02:45:54.9 -- not a known variable star
19:07:31.34 +01:49:27.4 -- not a known variable star
19:07:31.91 +02:47:51.9 -- not a known variable star
19:07:32.71 +01:50:08.0 -- not a known variable star
19:07:32.99 +02:13:42.1 -- not a known variable star
19:07:38.02 +01:53:34.9 -- not a known variable star
19:07:38.10 +02:03:28.3 -- not a known variable star
19:07:38.28 +03:00:46.9 -- a known variable star
19:07:38.79 +02:32:39.1 -- not a known variable star
19:07:39.63 +02:42:38.2 -- not a known variable star
19:07:39.68 +02:11:07.2 -- a known variable star
19:07:40.86 +02:47:19.4 -- not a known variable star
19:07:42.24 +01:51:56.2 -- not a known variable star
19:07:42.37 +01:47:57.2 -- not a known variable star
19:07:43.77 +01:56:52.6 -- not a known variable star
19:07:45.47 +01:59:16.1 -- not a known variable star
19:07:47.23 +02:03:36.6 -- not a known variable star
19:07:47.68 +02:02:07.7 -- a known variable star
19:07:48.23 +01:56:29.2 -- a known variable star
19:07:48.68 +02:01:05.7 -- not a known variable star
19:07:48.76 +02:05:56.0 -- a known variable star
19:07:51.72 +02:08:04.8 -- not a known variable star
19:07:52.14 +01:55:20.3 -- not a known variable star
19:07:53.71 +02:43:38.3 -- not a known variable star
19:07:54.13 +02:29:27.7 -- not a known variable star
19:07:55.27 +02:02:15.1 -- not a known variable star
19:07:56.31 +02:31:46.7 -- not a known variable star
19:07:57.26 +02:11:27.4 -- not a known variable star
19:07:58.92 +02:51:02.6 -- not a known variable star
19:07:59.70 +03:16:25.6 -- not a known variable star
19:08:00.01 +02:18:43.4 -- a known variable star
19:08:00.29 +02:38:46.5 -- not a known variable star
19:08:01.58 +03:04:56.0 -- a known variable star
19:08:02.39 +02:20:34.3 -- a known variable star
19:08:04.13 +03:04:09.4 -- not a known variable star
19:08:04.67 +01:55:53.5 -- not a known variable star
19:08:05.19 +02:16:24.4 -- not a known variable star
19:08:07.71 +02:09:14.4 -- not a known variable star
19:08:11.23 +02:44:50.7 -- not a known variable star
19:08:11.46 +02:05:51.0 -- not a known variable star
19:08:11.84 +02:38:41.4 -- not a known variable star
19:08:12.89 +02:21:06.3 -- not a known variable star
19:08:13.69 +02:33:15.2 -- a known variable star
19:08:14.46 +02:45:19.1 -- not a known variable star
19:08:14.48 +02:37:27.0 -- a known variable star
19:08:16.80 +03:16:51.9 -- not a known variable star
19:08:22.00 +03:12:18.8 -- not a known variable star
19:08:23.22 +02:21:10.7 -- not a known variable star
19:08:24.18 +02:53:37.2 -- not a known variable star
19:08:24.76 +03:07:17.8 -- not a known variable star
19:08:26.37 +02:59:04.3 -- not a known variable star
19:08:27.62 +03:22:42.3 -- a known variable star
19:08:31.82 +02:19:12.8 -- not a known variable star
19:08:33.03 +02:46:56.7 -- a known variable star
19:08:44.66 +02:29:02.4 -- not a known variable star
19:08:45.19 +02:40:45.7 -- a known variable star
19:08:59.06 +02:28:18.8 -- not a known variable star
19:08:59.41 +02:20:11.8 -- not a known variable star
19:09:06.51 +02:34:27.6 -- not a known variable star
Found 88 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
106 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 106 (excluding asteroids and hot pixels, 88 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)2461186.69815626 -observatory V36
05:07:20.01 +24:43:27.4 Mercury (-1.1mag)
06:35:58.87 +24:58:57.2 Venus (-3.9mag)
02:12:05.71 +12:34:05.7 Mars (1.3mag)
07:37:59.82 +21:56:24.2 Jupiter (-1.9mag)
00:45:18.33 +02:25:54.6 Saturn (0.9mag)
03:57:04.35 +20:16:19.4 Uranus (5.8mag)
00:15:13.79 +00:11:34.1 Neptune (7.8mag)
20:33:56.24 -23:00:04.1 Pluto (14.5mag)
12:20:10.29 -05:51:38.9 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 25 23:51 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461186.69815626:
07:37:54.86 +21:56:36.7 Io (5.9mag)
07:38:10.29 +21:55:54.3 Europa (6.1mag)
07:37:52.83 +21:56:48.6 Ganymede (5.5mag)
07:37:37.98 +21:57:17.7 Callisto (6.7mag)
07:39:04.88 +21:32:44.7 Himalia (15.5mag)
07:38:00.48 +21:56:23.8 Thebe (16.5mag)
07:39:23.22 +21:53:59.8 Elara (17.5mag)
07:39:27.66 +22:15:08.9 Pasiphae (17.7mag)
07:45:06.90 +21:57:13.8 Carme (18.8mag)
00:45:20.52 +02:25:34.9 Titan (8.7mag)
00:45:14.32 +02:26:02.4 Rhea (10.0mag)
00:45:41.03 +02:26:01.6 Iapetus (11.4mag)
00:45:33.07 +02:25:57.6 Hyperion (14.7mag)
00:46:15.96 +02:29:41.5 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 23:51 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.69815626:
17:17:23.12 -33:20:50.8 JWST
16:04:50.85 +52:08:33.6 Chandra
08:20:57.27 -45:06:10.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 23:51 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.69815626 -observatory V36
13:20:46.15 -27:03:31.4 14.4mag D/1884 O1 (Barnard)
06:37:23.92 +30:40:17.9 15.7mag D/1886 K1 (Brooks)
15:26:16.84 +01:21:00.1 14.6mag D/1895 Q1 (Swift)
05:28:12.21 +24:38:56.5 17.2mag D/1918 W1 (Schorr)
09:31:28.71 +14:31:57.6 17.9mag P/2009 WX51 (Catalina)
18:51:00.64 -31:39:30.4 13.7mag P/2010 H2 (Vales)
05:40:53.91 -68:16:01.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:21.67 +31:48:30.7 17.4mag C/2017 K2 (PANSTARRS)
17:19:51.32 +14:33:00.6 17.7mag C/2021 G2 (ATLAS)
23:14:32.78 +31:02:51.9 17.2mag C/2022 E2 (ATLAS)
05:18:01.73 +26:51:29.1 16.4mag C/2022 N2 (PANSTARRS)
09:20:58.38 +31:29:34.6 16.5mag C/2022 QE78 (ATLAS)
08:44:01.54 +03:13:09.9 17.6mag C/2022 R6 (PANSTARRS)
18:36:21.15 +21:12:19.1 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:26.59 -11:02:16.0 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.45 +65:39:49.5 17.7mag C/2023 H5 (Lemmon)
18:17:04.02 -05:32:13.9 13.7mag C/2023 R1 (PANSTARRS)
13:39:44.73 +85:47:50.7 17.9mag C/2023 X2 (Lemmon)
06:53:27.21 +63:55:43.7 17.6mag C/2024 A1 (ATLAS)
06:26:54.78 +26:29:00.4 13.1mag C/2024 E1 (Wierzchos)
15:47:52.18 +12:12:39.3 17.3mag C/2024 G6 (ATLAS)
20:19:47.55 +27:10:44.5 14.1mag C/2024 J3 (ATLAS)
04:04:59.91 -17:12:08.6 16.1mag C/2024 T5 (ATLAS)
05:53:40.50 +36:48:43.4 17.9mag C/2025 J1 (Borisov)
11:45:40.41 +53:20:11.1 16.9mag C/2025 L1 (ATLAS)
06:24:57.24 -10:11:21.8 12.6mag C/2025 R3 (PANSTARRS)
12:40:57.04 +04:36:59.9 17.2mag C/2025 Y1 (ATLAS)
01:36:20.94 +42:23:01.3 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.45 -08:58:49.1 16.3mag A/2026 E1
19:59:41.98 -08:07:25.4 9.5mag 10P/Tempel
14:18:45.01 -02:35:32.8 17.6mag 24P/Schaumasse
10:59:43.26 -00:51:55.2 15.9mag 29P/Schwassmann-Wachmann
10:51:19.81 -02:34:28.6 17.8mag 43P/Wolf-Harrington
02:51:29.14 +23:50:18.3 17.6mag 47P/Ashbrook-Jackson
08:32:16.82 +27:21:50.4 16.9mag 63P/Wild
00:14:54.05 -07:19:15.4 15.7mag 65P/Gunn
06:01:41.66 +31:41:16.6 16.5mag 76P/West-Kohoutek-Ikemura
02:38:00.20 +15:23:34.0 13.9mag 78P/Gehrels
00:51:11.48 +01:49:25.4 15.3mag 88P/Howell
04:12:49.43 +28:56:48.4 15.1mag 93P/Lovas
02:07:27.54 +25:21:22.8 17.9mag 114P/Wiseman-Skiff
06:20:01.88 +33:19:27.1 15.7mag 123P/West-Hartley
09:27:59.06 +20:15:43.7 16.4mag 124P/Mrkos
03:37:37.78 +18:17:26.4 16.4mag 128P/Shoemaker-Holt
04:07:36.26 +18:20:57.9 17.7mag 131P/Mueller
04:58:46.88 +19:38:40.5 13.0mag 141P/Machholz
05:01:25.56 +16:23:04.2 12.9mag 141P-A/Machholz
03:46:36.23 +13:43:19.5 10.6mag 141P-D/Machholz
02:48:12.58 -26:39:03.6 17.3mag 161P/Hartley-IRAS
02:59:57.02 +18:14:23.8 14.9mag 162P/SidingSpring
19:34:45.27 -01:42:27.1 17.6mag 169P/NEAT
17:02:20.54 -09:21:27.6 16.2mag 235P/LINEAR
07:05:04.22 +35:51:51.8 17.3mag 240P/NEAT
23:58:35.71 -07:45:51.3 16.7mag 260P/McNaught
03:30:02.69 +29:55:34.1 17.7mag 295P/LINEAR
22:05:24.50 -27:29:11.7 17.7mag 320P/McNaught
15:21:44.23 +08:21:36.8 17.4mag 391P/Kowalski
07:57:13.87 +21:02:17.9 17.8mag 450P/LONEOS
06:38:47.05 +42:35:10.5 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 23:51 comets.txt
############################################################
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 23:51 asassn_transients_list.txt
############################################################
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 23:51 tocp_transients_list.txt
############################################################
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 23:51 tns_transients_list.txt
