This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Lyr-02-Q2b1x1_015244_TTUQ2b1x1_2008450_VVGKEclE
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.05 18:26:57.73 +37:09:48.1
65.12741 20.55189 galactic Lyr Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:57.73 +37:09:48.1 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:57.73 +37:09:48.1: 12.95 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:57.73 +37:09:48.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.70 18:17:16.34 +36:53:47.6
64.19586 22.30090 galactic Lyr Second-epoch detections are separated by 1.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:16.34 +36:53:47.6 (user input) | T | P | (position from user input) J-Ks=0.712+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:16.34 +36:53:47.6: 14.27 +/- 0.07 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:16.34 +36:53:47.6: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.44 18:20:29.47 +35:43:37.3
63.22070 21.31674 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.1383+35.7267 | 18:20:29.47 +35:43:37.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.409+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:29.47 +35:43:37.3: 13.83 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:29.47 +35:43:37.3: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 J275.1383+35.7267,2461239.7595,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.1383+35.7267 20260718.2595 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.00 18:26:30.95 +36:58:23.7
64.90443 20.57387 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:30.95 +36:58:23.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.711+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:30.95 +36:58:23.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:30.95 +36:58:23.7: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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
target,2461239.7595,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.56 18:27:47.76 +36:34:36.4
64.59521 20.20119 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2095832306878604800 | 18:27:47.79 +36:34:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.626+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:47.76 +36:34:36.4: 12.48 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:47.76 +36:34:36.4: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 2095832306878604800,2461239.7595,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2095832306878604800 20260718.2595 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 07 18.2595 2461239.7595 12.62 18:21:38.39 +35:22:32.0
62.94551 20.98170 galactic Lyr Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:38.39 +35:22:32.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.641+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:38.39 +35:22:32.0: 14.06 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:38.39 +35:22:32.0: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.04 +/- 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
target,2461239.7595,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.61 18:19:18.84 +35:15:31.9
62.66190 21.39255 galactic Lyr Second-epoch detections are separated by 1.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:18.84 +35:15:31.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.427+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:18.84 +35:15:31.9: 13.87 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:18.84 +35:15:31.9: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 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
target,2461239.7595,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.19 18:22:54.85 +36:00:21.0
63.67392 20.94259 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:54.85 +36:00:21.0 (user input) | T | P | (position from user input) J-Ks=0.293+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:54.85 +36:00:21.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:54.85 +36:00:21.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
target,2461239.7595,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.83 18:18:59.79 +36:30:15.6
63.90978 21.85035 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:59.79 +36:30:15.6 (user input) | T | P | (position from user input) J-Ks=0.284+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:59.79 +36:30:15.6: 12.99 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:59.79 +36:30:15.6: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.38 18:17:36.21 +36:45:23.8
64.07420 22.19461 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.4017+36.7587 | 18:17:36.20 +36:45:24.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.285+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:36.21 +36:45:23.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:36.21 +36:45:23.8: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 J274.4017+36.7587,2461239.7595,11.38,0.05,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 J274.4017+36.7587 20260718.2595 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.89 18:20:36.82 +35:07:35.9
62.62015 21.09848 galactic Lyr Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593633347465865216 | 18:20:36.82 +35:07:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:36.82 +35:07:35.9: 11.89 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:36.82 +35:07:35.9: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 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
Gaia DR3 4593633347465865216,2461239.7595,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4593633347465865216 20260718.2595 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:17:54.65 +36:47:19.7
64.12786 22.14609 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was found in VSX 0" Gaia DR3 4606032849332700416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.430 G 13.460 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:54.65 +36:47:19.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:54.65 +36:47:19.7: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 4606032849332700416,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606032849332700416 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.45 18:13:41.80 +37:57:28.6
65.06192 23.29741 galactic Her Second-epoch detections are separated by 1.3" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.4181+37.9642 | 18:13:41.80 +37:57:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.618+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:13:41.80 +37:57:28.6: 13.36 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:13:41.80 +37:57:28.6: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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!
TCP 2026 07 18.2595* 18 13 41.80 +37 57 28.6 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.4181+37.9642,2461239.7595,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.4181+37.9642 20260718.2595 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.03 18:16:47.46 +36:50:30.6
64.10751 22.37563 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:47.46 +36:50:30.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.376+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:47.46 +36:50:30.6: 13.37 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:47.46 +36:50:30.6: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
target,2461239.7595,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.41 18:32:54.76 +39:03:22.7
67.44334 20.06646 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:32:54.76 +39:03:22.7 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:32:54.76 +39:03:22.7: 13.63 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:32:54.76 +39:03:22.7: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 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
target,2461239.7595,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.62 18:26:45.08 +36:52:48.1
64.82684 20.49887 galactic Lyr Second-epoch detections are separated by 1.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:45.08 +36:52:48.1 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:45.08 +36:52:48.1: 13.90 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:45.08 +36:52:48.1: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.13 18:21:06.43 +35:05:07.3
62.61369 20.98961 galactic Lyr Second-epoch detections are separated by 0.6" and 2.3 pix
The object was found in VSX 1" Gaia DR3 4593629396098885760
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.220 G 13.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:06.43 +35:05:07.3: 13.39 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:06.43 +35:05:07.3: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4593629396098885760,2461239.7595,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4593629396098885760 20260718.2595 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.89 18:20:25.35 +34:59:41.3
62.47290 21.09244 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:25.35 +34:59:41.3 (user input) | T | P | (position from user input) J-Ks=0.833+/-0.028 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:25.35 +34:59:41.3: 13.02 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:25.35 +34:59:41.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.12 18:20:54.04 +35:55:49.0
63.45593 21.30361 galactic Lyr Second-epoch detections are separated by 2.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2283+35.9268 | 18:20:54.04 +35:55:49.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.568+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:54.04 +35:55:49.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:54.04 +35:55:49.0: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.2283+35.9268,2461239.7595,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.2283+35.9268 20260718.2595 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.74 18:20:47.00 +36:05:52.4
63.61817 21.37992 galactic Lyr Second-epoch detections are separated by 1.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.1997+36.1102 | 18:20:47.00 +36:05:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.760+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:47.00 +36:05:52.4: 13.03 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:47.00 +36:05:52.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.1997+36.1102,2461239.7595,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.1997+36.1102 20260718.2595 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.32 18:20:01.37 +36:18:36.7
63.78178 21.59307 galactic Lyr Second-epoch detections are separated by 1.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:01.37 +36:18:36.7 (user input) | T | P | (position from user input) J-Ks=0.294+/-0.032 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:01.37 +36:18:36.7: 13.44 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:01.37 +36:18:36.7: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.76 18:26:09.97 +36:58:52.6
64.88816 20.64250 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.5441+36.9839 | 18:26:09.91 +36:58:52.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.751+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:09.97 +36:58:52.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:09.97 +36:58:52.6: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 J276.5441+36.9839,2461239.7595,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.5441+36.9839 20260718.2595 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.04 18:26:03.15 +37:37:41.7
65.53483 20.87367 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:03.15 +37:37:41.7 (user input) | T | P | (position from user input) J-Ks=0.277+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:03.15 +37:37:41.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:03.15 +37:37:41.7: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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,2461239.7595,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:25:56.89 +37:04:27.0
64.96688 20.71390 galactic Lyr Second-epoch detections are separated by 1.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:56.89 +37:04:27.0 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.031 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:56.89 +37:04:27.0: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:56.89 +37:04:27.0: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.38 18:20:02.39 +35:15:47.5
62.71776 21.25375 galactic Lyr Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:02.39 +35:15:47.5 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:02.39 +35:15:47.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:02.39 +35:15:47.5: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461239.7595,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:19:59.42 +35:56:26.6
63.40305 21.48149 galactic Lyr Second-epoch detections are separated by 1.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:59.42 +35:56:26.6 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:59.42 +35:56:26.6: 13.46 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:59.42 +35:56:26.6: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
target,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.57 18:13:33.91 +37:31:28.1
64.60280 23.19434 galactic Her Second-epoch detections are separated by 3.4" and 1.6 pix
The object was found in VSX24" Gaia DR3 4606886688830952704
Type: E
# Max. Min./Amp. JD0 Period
15.040 G 15.160 G 3.089790000000 G
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:13:33.91 +37:31:28.1: 13.45 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:13:33.91 +37:31:28.1: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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!
TCP 2026 07 18.2595* 18 13 33.91 +37 31 28.1 12.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4606886688830952704,2461239.7595,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606886688830952704 20260718.2595 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.31 18:26:56.02 +36:37:39.4
64.58528 20.38133 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:56.02 +36:37:39.4 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.026 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:56.02 +36:37:39.4: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:56.02 +36:37:39.4: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.13 18:28:25.53 +36:15:34.4
64.32175 19.97600 galactic Lyr Second-epoch detections are separated by 1.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:28:25.53 +36:15:34.4 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:28:25.53 +36:15:34.4: 13.09 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:28:25.53 +36:15:34.4: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.02 18:16:26.75 +36:45:38.6
64.00105 22.41642 galactic Lyr Second-epoch detections are separated by 1.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:26.75 +36:45:38.6 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:26.75 +36:45:38.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:26.75 +36:45:38.6: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:14:15.76 +37:22:54.7
64.49958 23.01974 galactic Her Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.5512+37.3770 | 18:14:15.76 +37:22:54.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.352+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:14:15.76 +37:22:54.7: 13.48 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:14:15.76 +37:22:54.7: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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!
TCP 2026 07 18.2595* 18 14 15.76 +37 22 54.7 12.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.5512+37.3770,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.5512+37.3770 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.89 18:17:24.41 +36:43:56.8
64.03619 22.22458 galactic Lyr Second-epoch detections are separated by 1.9" and 1.9 pix
The object was found in VSX 1" Gaia DR3 4606031749820917632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.130 G 14.160 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:24.41 +36:43:56.8: 14.37 +/- 0.07 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:24.41 +36:43:56.8: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4606031749820917632,2461239.7595,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606031749820917632 20260718.2595 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:38:07.84 +37:38:16.8
66.39568 18.62389 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:38:07.84 +37:38:16.8 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.034 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:38:07.84 +37:38:16.8: 13.13 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:38:07.84 +37:38:16.8: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.07 18:20:36.57 +36:17:20.7
63.80072 21.47430 galactic Lyr Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:36.57 +36:17:20.7 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:36.57 +36:17:20.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:36.57 +36:17:20.7: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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,2461239.7595,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.08 18:21:40.01 +35:09:46.6
62.73233 20.90690 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:40.01 +35:09:46.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.762+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:40.01 +35:09:46.6: 13.15 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:40.01 +35:09:46.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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,2461239.7595,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.52 18:24:06.76 +37:13:19.9
64.99041 21.10786 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:24:06.76 +37:13:19.9 (user input) | T | P | (position from user input) J-Ks=0.333+/-0.034 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:24:06.76 +37:13:19.9: 13.70 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:24:06.76 +37:13:19.9: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.05 18:19:48.26 +36:08:50.6
63.60071 21.58307 galactic Lyr Second-epoch detections are separated by 1.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:48.26 +36:08:50.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.429+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:48.26 +36:08:50.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:48.26 +36:08:50.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 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,2461239.7595,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.67 18:20:48.09 +35:43:33.7
63.24148 21.25680 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2038+35.7271 | 18:20:48.09 +35:43:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.318+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:48.09 +35:43:33.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:48.09 +35:43:33.7: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J275.2038+35.7271,2461239.7595,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.2038+35.7271 20260718.2595 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.50 18:26:04.39 +37:34:52.4
65.48860 20.85463 galactic Lyr Second-epoch detections are separated by 1.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:04.39 +37:34:52.4 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.306+/-0.032 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:04.39 +37:34:52.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:04.39 +37:34:52.4: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
target,2461239.7595,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:26:36.99 +36:57:29.7
64.89632 20.54996 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:36.99 +36:57:29.7 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:36.99 +36:57:29.7: 13.17 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:36.99 +36:57:29.7: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.40 18:20:23.73 +36:25:30.8
63.92469 21.55849 galactic Lyr Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0957+36.4275 | 18:20:23.73 +36:25:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.577+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:23.73 +36:25:30.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:23.73 +36:25:30.8: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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 J275.0957+36.4275,2461239.7595,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0957+36.4275 20260718.2595 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.21 18:21:11.00 +35:13:38.5
62.76289 21.02133 galactic Lyr Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2958+35.2273 | 18:21:11.00 +35:13:38.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.027 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:11.00 +35:13:38.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:11.00 +35:13:38.5: 12.14 +/- 0.01 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 J275.2958+35.2273,2461239.7595,11.21,0.05,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
ATO J275.2958+35.2273 20260718.2595 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.60 18:17:17.28 +36:50:22.7
64.13839 22.28036 galactic Lyr Second-epoch detections are separated by 1.4" and 2.0 pix
The object was found in VSX 1" ZTF J181717.30+365023.5
Type: EB
# Max. Min./Amp. JD0 Period
14.446 g Y 0.166 g 2458258.84190 5.567689600000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:17.28 +36:50:22.7: 13.96 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:17.28 +36:50:22.7: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 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
ZTF J181717.30+365023.5,2461239.7595,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J181717.30+365023.5 20260718.2595 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.65 18:22:17.09 +36:00:29.1
63.63192 21.06369 galactic Lyr Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:17.09 +36:00:29.1 (user input) | T | P | (position from user input) J-Ks=0.570+/-0.025 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:17.09 +36:00:29.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:17.09 +36:00:29.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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
target,2461239.7595,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.26 18:22:44.76 +35:34:27.0
63.22529 20.83386 galactic Lyr Second-epoch detections are separated by 1.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:44.76 +35:34:27.0 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.303+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:44.76 +35:34:27.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:44.76 +35:34:27.0: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.94 18:28:25.39 +37:15:31.4
65.32539 20.30840 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:28:25.39 +37:15:31.4 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:28:25.39 +37:15:31.4: 12.80 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:28:25.39 +37:15:31.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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
target,2461239.7595,11.94,0.05,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
target 20260718.2595 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.47 18:16:34.78 +36:56:15.8
64.19218 22.44530 galactic Lyr Second-epoch detections are separated by 1.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:34.78 +36:56:15.8 (user input) | T | P | (position from user input) J-Ks=0.497+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:34.78 +36:56:15.8: 13.73 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:34.78 +36:56:15.8: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.42 18:25:36.73 +37:24:42.1
65.28530 20.88650 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:36.73 +37:24:42.1 (user input) | T | P | (position from user input) J-Ks=0.194+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:36.73 +37:24:42.1: 13.73 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:36.73 +37:24:42.1: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461239.7595,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.50 18:19:03.60 +36:33:07.4
63.96291 21.85324 galactic Lyr Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:03.60 +36:33:07.4 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:03.60 +36:33:07.4: 13.74 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:03.60 +36:33:07.4: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.33 18:16:33.62 +36:47:32.1
64.04112 22.40430 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.1353+36.7943 | 18:16:33.63 +36:47:32.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.026 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:33.62 +36:47:32.1: 12.30 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:33.62 +36:47:32.1: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 J274.1353+36.7943,2461239.7595,11.33,0.05,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
ATO J274.1353+36.7943 20260718.2595 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.62 18:16:28.94 +36:44:54.8
63.99096 22.40572 galactic Lyr Second-epoch detections are separated by 0.4" and 2.1 pix
The object was found in VSX 1" V0729 Lyr
Type: RRC
# Max. Min./Amp. JD0 Period
12.350 CV 12.800 CV 2454700.61400 0.297101000000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:28.94 +36:44:54.8: 12.83 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:28.94 +36:44:54.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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
V0729 Lyr,2461239.7595,11.62,0.05,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
V0729 Lyr 20260718.2595 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.08 18:16:52.13 +36:49:12.6
64.09040 22.35414 galactic Lyr Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.2213+36.8208 | 18:16:52.13 +36:49:12.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.422+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:52.13 +36:49:12.6: 13.25 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:52.13 +36:49:12.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 J274.2213+36.8208,2461239.7595,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.2213+36.8208 20260718.2595 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.19 18:21:58.83 +35:07:13.8
62.71196 20.83240 galactic Lyr Second-epoch detections are separated by 1.8" and 2.3 pix
The object was found in VSX11" ZTF J182159.68+350711.7
Type: EW
# Max. Min./Amp. JD0 Period
15.806 g Y 0.333 g 2458235.96330 0.381270800000
ATTENTION: measured mag 12.19 is 3.3 mag brighter than the VSX record maximum brightness 15.47 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:58.83 +35:07:13.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:58.83 +35:07:13.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J182159.68+350711.7,2461239.7595,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J182159.68+350711.7 20260718.2595 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.99 18:18:34.80 +36:32:53.2
63.92628 21.94354 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:34.80 +36:32:53.2 (user input) | T | P | (position from user input) J-Ks=0.263+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:34.80 +36:32:53.2: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:34.80 +36:32:53.2: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.26 18:18:19.52 +36:42:13.7
64.06855 22.04073 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605984844481616000 | 18:18:19.51 +36:42:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.403+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:19.52 +36:42:13.7: 12.35 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:19.52 +36:42:13.7: 12.28 +/- 0.01 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 4605984844481616000,2461239.7595,11.26,0.05,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 4605984844481616000 20260718.2595 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.26 18:16:35.00 +37:08:31.9
64.40308 22.50717 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:35.00 +37:08:31.9 (user input) | T | P | (position from user input) J-Ks=0.682+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:35.00 +37:08:31.9: 13.25 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:35.00 +37:08:31.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 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,2461239.7595,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.93 18:25:41.48 +37:36:35.3
65.49149 20.93544 galactic Lyr Second-epoch detections are separated by 1.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.4265+37.6073 | 18:25:41.48 +37:36:35.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.558+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:41.48 +37:36:35.3: 12.88 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:41.48 +37:36:35.3: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 J276.4265+37.6073,2461239.7595,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.4265+37.6073 20260718.2595 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.41 18:21:54.73 +34:56:11.3
62.52114 20.78500 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593613418820430976 | 18:21:54.73 +34:56:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.960+/-0.027 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:54.73 +34:56:11.3: 12.37 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:54.73 +34:56:11.3: 12.32 +/- 0.01 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 4593613418820430976,2461239.7595,11.41,0.05,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 4593613418820430976 20260718.2595 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 07 18.2595 2461239.7595 12.18 18:20:33.25 +35:49:00.3
63.31630 21.33354 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:33.25 +35:49:00.3 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:33.25 +35:49:00.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:33.25 +35:49:00.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.99 18:16:45.02 +36:54:47.1
64.17813 22.40527 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:45.02 +36:54:47.1 (user input) | T | P | (position from user input) J-Ks=0.664+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:45.02 +36:54:47.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:45.02 +36:54:47.1: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 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,2461239.7595,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.97 18:20:05.97 +35:20:47.7
62.80664 21.26925 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0262+35.3496 | 18:20:05.97 +35:20:47.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.421+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:05.97 +35:20:47.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:05.97 +35:20:47.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J275.0262+35.3496,2461239.7595,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0262+35.3496 20260718.2595 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.01 18:17:57.78 +36:46:05.5
64.11021 22.12976 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:57.78 +36:46:05.5 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:57.78 +36:46:05.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:57.78 +36:46:05.5: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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,2461239.7595,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.55 18:26:48.51 +37:30:11.4
65.46005 20.69145 galactic Lyr Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:48.51 +37:30:11.4 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:48.51 +37:30:11.4: 13.77 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:48.51 +37:30:11.4: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.37 18:19:27.19 +34:05:16.3
61.48484 20.98319 galactic Lyr Second-epoch detections are separated by 2.6" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:27.19 +34:05:16.3 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:27.19 +34:05:16.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:27.19 +34:05:16.3: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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,2461239.7595,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:16:54.48 +37:03:34.5
64.33941 22.42026 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was found in VSX 0" Gaia DR3 4606054770845887232
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.090 G 13.130 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:54.48 +37:03:34.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:54.48 +37:03:34.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4606054770845887232,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606054770845887232 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.71 18:19:48.94 +35:12:14.2
62.64169 21.27785 galactic Lyr Second-epoch detections are separated by 2.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:48.94 +35:12:14.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.716+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:48.94 +35:12:14.2: 14.19 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:48.94 +35:12:14.2: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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
target,2461239.7595,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.22 18:26:40.54 +36:34:19.4
64.51110 20.41189 galactic Lyr Second-epoch detections are separated by 1.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.6651+36.5729 | 18:26:40.54 +36:34:19.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.358+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:40.54 +36:34:19.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:40.54 +36:34:19.4: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.6651+36.5729,2461239.7595,12.22,0.05,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
ATO J276.6651+36.5729 20260718.2595 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.53 18:15:07.75 +37:16:07.9
64.43868 22.82150 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:15:07.75 +37:16:07.9 (user input) | T | P | (position from user input) J-Ks=0.702+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:07.75 +37:16:07.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:07.75 +37:16:07.9: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.40 18:17:32.96 +36:28:15.7
63.77747 22.11618 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.3832+36.4647 | 18:17:32.96 +36:28:15.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.310+/-0.032 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:32.96 +36:28:15.7: 13.80 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:32.96 +36:28:15.7: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.3832+36.4647,2461239.7595,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.3832+36.4647 20260718.2595 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:26:43.33 +37:15:35.8
65.20828 20.62858 galactic Lyr Second-epoch detections are separated by 2.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:43.33 +37:15:35.8 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:43.33 +37:15:35.8: 13.57 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:43.33 +37:15:35.8: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.54 18:26:06.96 +37:14:57.3
65.15554 20.73917 galactic Lyr Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:06.96 +37:14:57.3 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:06.96 +37:14:57.3: 13.81 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:06.96 +37:14:57.3: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.66 18:18:53.44 +36:02:17.5
63.42622 21.72339 galactic Lyr Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.7225+36.0383 | 18:18:53.44 +36:02:17.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.683+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:53.44 +36:02:17.5: 13.83 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:53.44 +36:02:17.5: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.7225+36.0383,2461239.7595,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.7225+36.0383 20260718.2595 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.55 18:25:27.50 +37:16:23.3
65.13438 20.87071 galactic Lyr Second-epoch detections are separated by 2.0" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:27.50 +37:16:23.3 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:27.50 +37:16:23.3: 13.81 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:27.50 +37:16:23.3: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.66 18:15:48.09 +37:12:21.0
64.41741 22.67489 galactic Lyr Second-epoch detections are separated by 1.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:15:48.09 +37:12:21.0 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:48.09 +37:12:21.0: 13.81 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:48.09 +37:12:21.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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
target,2461239.7595,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.59 18:20:04.91 +35:14:38.9
62.70140 21.23946 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was found in VSX 1" Gaia DR3 4605647539226060928
Type: ROT
# Max. Min./Amp. JD0 Period
13.570 G 13.600 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:04.91 +35:14:38.9: 13.81 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:04.91 +35:14:38.9: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4605647539226060928,2461239.7595,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605647539226060928 20260718.2595 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.51 18:17:33.42 +36:47:07.2
64.10058 22.21236 galactic Lyr Second-epoch detections are separated by 0.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606032299576929536 | 18:17:33.43 +36:47:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.705+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:33.42 +36:47:07.2: 11.44 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:33.42 +36:47:07.2: 11.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.42 +/- 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
Gaia DR3 4606032299576929536,2461239.7595,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606032299576929536 20260718.2595 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.52 18:19:11.28 +36:30:14.4
63.92248 21.81372 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.7950+36.5065 | 18:19:11.28 +36:30:14.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.449+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:11.28 +36:30:14.4: 13.81 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:11.28 +36:30:14.4: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.7950+36.5065,2461239.7595,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.7950+36.5065 20260718.2595 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.62 18:20:55.56 +35:10:33.8
62.69254 21.05426 galactic Lyr Second-epoch detections are separated by 1.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:55.56 +35:10:33.8 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:55.56 +35:10:33.8: 13.75 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:55.56 +35:10:33.8: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.69 18:18:16.08 +36:37:46.4
63.98858 22.02849 galactic Lyr Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:16.08 +36:37:46.4 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:16.08 +36:37:46.4: 14.02 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:16.08 +36:37:46.4: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
target,2461239.7595,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.44 18:21:34.99 +35:37:40.3
63.19704 21.07482 galactic Lyr Second-epoch detections are separated by 0.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605679906100024960 | 18:21:34.99 +35:37:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:34.99 +35:37:40.3: 12.44 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:34.99 +35:37:40.3: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 4605679906100024960,2461239.7595,11.44,0.05,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 4605679906100024960 20260718.2595 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.39 18:20:55.76 +35:45:50.3
63.28900 21.24450 galactic Lyr Second-epoch detections are separated by 0.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605697085969252992 | 18:20:55.74 +35:45:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.810+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:55.76 +35:45:50.3: 12.44 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:55.76 +35:45:50.3: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 4605697085969252992,2461239.7595,11.39,0.05,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 4605697085969252992 20260718.2595 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.83 18:18:38.25 +36:37:42.2
64.01237 21.95771 galactic Lyr Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:38.25 +36:37:42.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.327+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:38.25 +36:37:42.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:38.25 +36:37:42.2: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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
target,2461239.7595,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.48 18:20:05.29 +35:28:00.2
62.92785 21.31029 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605663134249397760 | 18:20:05.31 +35:28:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:05.29 +35:28:00.2: 12.44 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:05.29 +35:28:00.2: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 4605663134249397760,2461239.7595,11.48,0.05,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
Gaia DR3 4605663134249397760 20260718.2595 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.38 18:16:14.04 +36:50:13.6
64.06562 22.48024 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:14.04 +36:50:13.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.272+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:14.04 +36:50:13.6: 13.29 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:14.04 +36:50:13.6: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.34 18:22:28.74 +35:48:07.7
63.43696 20.95959 galactic Lyr Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:28.74 +35:48:07.7 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.287+/-0.042 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:28.74 +35:48:07.7: 13.55 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:28.74 +35:48:07.7: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.44 18:20:22.59 +35:58:12.7
63.45994 21.41690 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605750304904931840 | 18:20:22.62 +35:58:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:22.59 +35:58:12.7: 12.43 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:22.59 +35:58:12.7: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 4605750304904931840,2461239.7595,11.44,0.05,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 4605750304904931840 20260718.2595 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.60 18:17:17.24 +36:42:08.8
63.99737 22.23806 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:17.24 +36:42:08.8 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:17.24 +36:42:08.8: 13.79 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:17.24 +36:42:08.8: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
target,2461239.7595,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.28 18:22:06.80 +35:57:17.6
63.56594 21.07927 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:06.80 +35:57:17.6 (user input) | T | P | (position from user input) J-Ks=0.556+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:06.80 +35:57:17.6: 13.56 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:06.80 +35:57:17.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 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,2461239.7595,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:26:43.57 +36:59:14.0
64.93321 20.53875 galactic Lyr Second-epoch detections are separated by 1.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2107867148838572288 | 18:26:43.57 +36:59:14.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F7 (LAMOST DR5) J-Ks=0.294+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:43.57 +36:59:14.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:43.57 +36:59:14.0: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 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
Large-amplitude variable Gaia DR2 2107867148838572288,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2107867148838572288 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.26 18:22:21.77 +34:54:00.4
62.51708 20.68580 galactic Lyr Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:21.77 +34:54:00.4 (user input) | T | P | (position from user input) J-Ks=0.666+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:21.77 +34:54:00.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:21.77 +34:54:00.4: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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
target,2461239.7595,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.61 18:19:30.44 +35:01:38.3
62.44043 21.28020 galactic Lyr Second-epoch detections are separated by 2.0" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:30.44 +35:01:38.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.482+/-0.031 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:30.44 +35:01:38.3: 13.78 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:30.44 +35:01:38.3: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
target,2461239.7595,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.44 18:21:07.98 +35:46:37.9
63.31674 21.20968 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605696772433274752 | 18:21:07.98 +35:46:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.629+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:07.98 +35:46:37.9: 12.41 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:07.98 +35:46:37.9: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 4605696772433274752,2461239.7595,11.44,0.05,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 4605696772433274752 20260718.2595 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.95 18:15:38.00 +37:10:50.0
64.38030 22.69914 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:15:38.00 +37:10:50.0 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:38.00 +37:10:50.0: 12.91 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:38.00 +37:10:50.0: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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
target,2461239.7595,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.44 18:16:57.91 +36:56:40.3
64.22476 22.37408 galactic Lyr Second-epoch detections are separated by 0.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606049616885081856 | 18:16:57.93 +36:56:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.632+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:57.91 +36:56:40.3: 12.41 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:57.91 +36:56:40.3: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 4606049616885081856,2461239.7595,11.44,0.05,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 4606049616885081856 20260718.2595 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.20 18:26:25.54 +37:25:40.5
65.35760 20.73890 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:25.54 +37:25:40.5 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:25.54 +37:25:40.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:25.54 +37:25:40.5: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.52 18:18:43.97 +36:27:44.8
63.84898 21.88750 galactic Lyr Second-epoch detections are separated by 1.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:43.97 +36:27:44.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:43.97 +36:27:44.8: 13.78 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:43.97 +36:27:44.8: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.42 18:23:08.03 +35:49:54.8
63.51344 20.84381 galactic Lyr Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:23:08.03 +35:49:54.8 (user input) | T | P | (position from user input) J-Ks=0.630+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:08.03 +35:49:54.8: 13.55 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:23:08.03 +35:49:54.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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
target,2461239.7595,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:20:24.01 +36:09:20.1
63.65029 21.47169 galactic Lyr Second-epoch detections are separated by 2.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:24.01 +36:09:20.1 (user input) | T | P | (position from user input) J-Ks=0.637+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:24.01 +36:09:20.1: 13.56 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:24.01 +36:09:20.1: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.40 18:20:19.59 +35:15:32.3
62.73385 21.19703 galactic Lyr Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0781+35.2573 | 18:20:19.59 +35:15:32.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.359+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:19.59 +35:15:32.3: 13.58 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:19.59 +35:15:32.3: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
ATO J275.0781+35.2573,2461239.7595,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0781+35.2573 20260718.2595 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.35 18:15:22.99 +37:18:15.1
64.49176 22.78399 galactic Lyr Second-epoch detections are separated by 0.8" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:15:22.99 +37:18:15.1 (user input) | T | P | (position from user input) J-Ks=0.662+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:22.99 +37:18:15.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:22.99 +37:18:15.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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
target,2461239.7595,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.13 18:22:56.36 +35:56:58.7
63.61880 20.91948 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.7451+35.9487 | 18:22:56.36 +35:56:58.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.551+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:56.36 +35:56:58.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:56.36 +35:56:58.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 J275.7451+35.9487,2461239.7595,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.7451+35.9487 20260718.2595 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.27 18:26:55.22 +37:08:05.7
65.09579 20.55047 galactic Lyr Second-epoch detections are separated by 1.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:55.22 +37:08:05.7 (user input) | T | P | (position from user input) J-Ks=12.318+/- (unrealisitic color!)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:55.22 +37:08:05.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:55.22 +37:08:05.7: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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
target,2461239.7595,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.04 18:21:56.21 +36:31:39.2
64.13507 21.29748 galactic Lyr Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.4739+36.5345 | 18:21:56.21 +36:31:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.606+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:56.21 +36:31:39.2: 12.91 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:56.21 +36:31:39.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 J275.4739+36.5345,2461239.7595,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.4739+36.5345 20260718.2595 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.28 18:20:15.59 +35:01:33.2
62.49275 21.13407 galactic Lyr Second-epoch detections are separated by 1.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:15.59 +35:01:33.2 (user input) | T | P | (position from user input) J-Ks=0.579+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:15.59 +35:01:33.2: 13.54 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:15.59 +35:01:33.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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
target,2461239.7595,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.32 18:12:31.18 +38:16:08.6
65.31279 23.60953 galactic Her Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:12:31.18 +38:16:08.6 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:31.18 +38:16:08.6: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:12:31.18 +38:16:08.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.2595* 18 12 31.18 +38 16 08.6 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.04 18:27:47.72 +36:09:51.1
64.18083 20.06386 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:47.72 +36:09:51.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.426+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:47.72 +36:09:51.1: 12.90 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:47.72 +36:09:51.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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
target,2461239.7595,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.92 18:22:02.51 +35:13:38.4
62.82434 20.85566 galactic Lyr Second-epoch detections are separated by 0.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:02.51 +35:13:38.4 (user input) | T | P | (position from user input) J-Ks=0.292+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:02.51 +35:13:38.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:02.51 +35:13:38.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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
target,2461239.7595,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.81 18:15:56.36 +36:57:03.1
64.16334 22.57113 galactic Lyr Second-epoch detections are separated by 1.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.9714+36.9565 | 18:15:56.36 +36:57:03.1 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.533+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:56.36 +36:57:03.1: 12.87 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:56.36 +36:57:03.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 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
ATO J273.9714+36.9565,2461239.7595,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.9714+36.9565 20260718.2595 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.71 18:20:44.69 +34:59:48.5
62.49805 21.03070 galactic Lyr Second-epoch detections are separated by 0.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:44.69 +34:59:48.5 (user input) | T | P | (position from user input) J-Ks=0.273+/-0.027 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:44.69 +34:59:48.5: 12.87 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:44.69 +34:59:48.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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
target,2461239.7595,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.73 18:20:12.76 +35:03:37.0
62.52423 21.15440 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0497+35.0566 | 18:20:12.77 +35:03:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.819+/-0.028 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:12.76 +35:03:37.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:12.76 +35:03:37.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 J275.0497+35.0566,2461239.7595,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0497+35.0566 20260718.2595 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.72 18:20:55.49 +35:46:50.2
63.30558 21.25074 galactic Lyr Second-epoch detections are separated by 0.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:55.49 +35:46:50.2 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:55.49 +35:46:50.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:55.49 +35:46:50.2: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.72,0.05,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
target 20260718.2595 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 07 18.2595 2461239.7595 12.54 18:20:02.08 +35:34:42.9
63.03775 21.35669 galactic Lyr Second-epoch detections are separated by 2.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:02.08 +35:34:42.9 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:02.08 +35:34:42.9: 13.76 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:02.08 +35:34:42.9: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461239.7595,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.46 18:20:16.40 +35:10:53.1
62.65140 21.18210 galactic Lyr Second-epoch detections are separated by 1.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:16.40 +35:10:53.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.746+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:16.40 +35:10:53.1: 13.76 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:16.40 +35:10:53.1: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461239.7595,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:19:58.80 +35:52:40.9
63.33851 21.46340 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was found in VSX 2" Gaia DR3 4605743402896346880
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.130 G 13.160 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:58.80 +35:52:40.9: 13.25 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:58.80 +35:52:40.9: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 4605743402896346880,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605743402896346880 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.62 18:19:35.15 +35:11:24.0
62.61121 21.31775 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:35.15 +35:11:24.0 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:35.15 +35:11:24.0: 13.75 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:35.15 +35:11:24.0: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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
target,2461239.7595,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.53 18:27:38.95 +36:52:32.1
64.88539 20.32785 galactic Lyr Second-epoch detections are separated by 0.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:38.95 +36:52:32.1 (user input) | T | P | (position from user input) J-Ks=0.869+/-0.027 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:38.95 +36:52:32.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:38.95 +36:52:32.1: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
target,2461239.7595,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.32 18:21:18.87 +35:03:38.1
62.60350 20.94141 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593628635886667008 | 18:21:18.88 +35:03:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.488+/-0.031 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:18.87 +35:03:38.1: 12.33 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:18.87 +35:03:38.1: 12.30 +/- 0.01 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 4593628635886667008,2461239.7595,11.32,0.05,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 4593628635886667008 20260718.2595 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.66 18:20:58.35 +36:10:37.0
63.71173 21.36908 galactic Lyr Second-epoch detections are separated by 0.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:58.35 +36:10:37.0 (user input) | T | P | (position from user input) J-Ks=0.690+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:58.35 +36:10:37.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:58.35 +36:10:37.0: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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
target,2461239.7595,11.66,0.05,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
target 20260718.2595 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 07 18.2595 2461239.7595 11.87 18:26:22.68 +37:25:58.6
65.35941 20.74948 galactic Lyr Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.5900+37.4344 | 18:26:22.68 +37:25:58.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.565+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:22.68 +37:25:58.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:22.68 +37:25:58.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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
ATO J276.5900+37.4344,2461239.7595,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.5900+37.4344 20260718.2595 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.66 18:20:35.38 +36:10:32.0
63.68375 21.44183 galactic Lyr Second-epoch detections are separated by 1.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:35.38 +36:10:32.0 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:35.38 +36:10:32.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:35.38 +36:10:32.0: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.66,0.05,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
target 20260718.2595 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 07 18.2595 2461239.7595 12.71 18:19:56.00 +35:03:14.1
62.49783 21.20638 galactic Lyr Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9812+35.0510 | 18:19:56.00 +35:03:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.370+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:56.00 +35:03:14.1: 14.16 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:56.00 +35:03:14.1: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.9812+35.0510,2461239.7595,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9812+35.0510 20260718.2595 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.15 18:26:07.17 +37:28:48.5
65.38941 20.81330 galactic Lyr Second-epoch detections are separated by 1.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:07.17 +37:28:48.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.345+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:07.17 +37:28:48.5: 13.23 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:07.17 +37:28:48.5: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.41 18:19:37.36 +35:05:18.7
62.51079 21.27774 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9054+35.0888 | 18:19:37.36 +35:05:18.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.440+/-0.074 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:37.36 +35:05:18.7: 13.77 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:37.36 +35:05:18.7: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.9054+35.0888,2461239.7595,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9054+35.0888 20260718.2595 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.84 18:19:57.45 +36:14:17.2
63.70377 21.58264 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:57.45 +36:14:17.2 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:57.45 +36:14:17.2: 12.84 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:57.45 +36:14:17.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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
target,2461239.7595,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.80 18:21:44.02 +35:28:26.2
63.05180 20.99575 galactic Lyr Second-epoch detections are separated by 1.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:44.02 +35:28:26.2 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:44.02 +35:28:26.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:44.02 +35:28:26.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.43 18:26:50.38 +36:25:27.4
64.37393 20.33197 galactic Lyr Second-epoch detections are separated by 3.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:50.38 +36:25:27.4 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:50.38 +36:25:27.4: 13.53 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:50.38 +36:25:27.4: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
target,2461239.7595,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.29 18:20:14.77 +36:17:13.4
63.77357 21.54305 galactic Lyr Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0613+36.2894 | 18:20:14.77 +36:17:13.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.258+/-0.033 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:14.77 +36:17:13.4: 13.52 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:14.77 +36:17:13.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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
ATO J275.0613+36.2894,2461239.7595,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0613+36.2894 20260718.2595 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.13 18:21:39.39 +35:36:42.5
63.18596 21.05550 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.4138+35.6118 | 18:21:39.39 +35:36:42.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.716+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:39.39 +35:36:42.5: 13.23 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:39.39 +35:36:42.5: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 J275.4138+35.6118,2461239.7595,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.4138+35.6118 20260718.2595 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.33 18:20:58.88 +36:05:50.3
63.63135 21.34185 galactic Lyr Second-epoch detections are separated by 1.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:58.88 +36:05:50.3 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.037 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:58.88 +36:05:50.3: 13.80 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:58.88 +36:05:50.3: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 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,2461239.7595,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.27 18:19:39.78 +35:55:12.1
63.35921 21.53766 galactic Lyr Second-epoch detections are separated by 1.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9166+35.9090 | 18:19:39.78 +35:55:12.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:39.78 +35:55:12.1: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:39.78 +35:55:12.1: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 J274.9166+35.9090,2461239.7595,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9166+35.9090 20260718.2595 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.47 18:22:28.47 +35:30:41.5
63.14260 20.86553 galactic Lyr Second-epoch detections are separated by 0.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:28.47 +35:30:41.5 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:28.47 +35:30:41.5: 13.55 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:28.47 +35:30:41.5: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.87 18:20:05.05 +36:20:11.6
63.81288 21.58973 galactic Lyr Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:05.05 +36:20:11.6 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:05.05 +36:20:11.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:05.05 +36:20:11.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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
target,2461239.7595,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.51 18:16:20.70 +37:03:22.8
64.29887 22.52620 galactic Lyr Second-epoch detections are separated by 1.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:20.70 +37:03:22.8 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:20.70 +37:03:22.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:20.70 +37:03:22.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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,2461239.7595,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.52 18:26:38.99 +36:29:21.1
64.42582 20.38945 galactic Lyr Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:38.99 +36:29:21.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.368+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:38.99 +36:29:21.1: 13.53 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:38.99 +36:29:21.1: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461239.7595,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.13 18:19:07.29 +36:34:37.9
63.99281 21.84942 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:07.29 +36:34:37.9 (user input) | T | P | (position from user input) J-Ks=0.567+/-0.026 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:07.29 +36:34:37.9: 13.23 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:07.29 +36:34:37.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.76 18:19:59.20 +35:12:34.7
62.65963 21.24665 galactic Lyr Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9965+35.2099 | 18:19:59.20 +35:12:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:59.20 +35:12:34.7: 12.83 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:59.20 +35:12:34.7: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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
ATO J274.9965+35.2099,2461239.7595,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9965+35.2099 20260718.2595 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:26:10.02 +37:25:31.9
65.33739 20.78671 galactic Lyr Second-epoch detections are separated by 1.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.5333+37.4083 | 18:26:09.46 +37:24:45.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.543+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:10.02 +37:25:31.9: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:10.02 +37:25:31.9: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.5333+37.4083,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.5333+37.4083 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.88 18:22:11.65 +35:45:27.2
63.37167 20.99969 galactic Lyr Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:11.65 +35:45:27.2 (user input) | T | P | (position from user input) J-Ks=0.566+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:11.65 +35:45:27.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:11.65 +35:45:27.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.80 18:19:39.70 +35:05:43.0
62.52042 21.27239 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9054+35.0888 | 18:19:39.70 +35:05:43.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:39.70 +35:05:43.0: 12.82 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:39.70 +35:05:43.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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
ATO J274.9054+35.0888,2461239.7595,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9054+35.0888 20260718.2595 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.89 18:28:12.22 +36:17:47.5
64.34290 20.03050 galactic Lyr Second-epoch detections are separated by 1.7" and 2.5 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 J277.0521+36.3004 | 18:28:12.22 +36:17:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.259+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:28:12.22 +36:17:47.5: 12.74 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:28:12.22 +36:17:47.5: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.72 +/- 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
ATO J277.0521+36.3004,2461239.7595,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J277.0521+36.3004 20260718.2595 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.99 18:20:28.81 +36:08:37.9
63.64390 21.45264 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605756115999997824 | 18:20:31.45 +36:08:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.444+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:28.81 +36:08:37.9: 13.21 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:28.81 +36:08:37.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4605756115999997824,2461239.7595,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605756115999997824 20260718.2595 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.32 18:21:05.44 +35:34:18.6
63.10539 21.15131 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605676607564771456 | 18:21:05.46 +35:34:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.274+/-0.027 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:05.44 +35:34:18.6: 12.30 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:05.44 +35:34:18.6: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 4605676607564771456,2461239.7595,11.32,0.05,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 4605676607564771456 20260718.2595 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.89 18:16:38.63 +37:07:34.1
64.39052 22.49078 galactic Lyr Second-epoch detections are separated by 1.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:38.63 +37:07:34.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.614+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:38.63 +37:07:34.1: 12.83 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:38.63 +37:07:34.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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
target,2461239.7595,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.04 18:20:08.23 +35:05:07.3
62.54427 21.17717 galactic Lyr Second-epoch detections are separated by 0.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:08.23 +35:05:07.3 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:08.23 +35:05:07.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:08.23 +35:05:07.3: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.12 18:20:10.13 +35:36:44.6
63.08154 21.34176 galactic Lyr Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:10.13 +35:36:44.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.331+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:10.13 +35:36:44.6: 13.22 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:10.13 +35:36:44.6: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.46 18:23:48.96 +35:48:39.9
63.54087 20.70634 galactic Lyr Second-epoch detections are separated by 2.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:23:48.96 +35:48:39.9 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:48.96 +35:48:39.9: 13.53 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:23:48.96 +35:48:39.9: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 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
target,2461239.7595,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.38 18:21:20.68 +35:00:44.7
62.55696 20.91977 galactic Lyr Second-epoch detections are separated by 2.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:20.68 +35:00:44.7 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:20.68 +35:00:44.7: 13.74 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:20.68 +35:00:44.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.43 18:20:56.48 +35:10:45.4
62.69690 21.05235 galactic Lyr Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:56.48 +35:10:45.4 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:56.48 +35:10:45.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:56.48 +35:10:45.4: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.37 18:18:46.29 +36:31:17.3
63.91201 21.89866 galactic Lyr Second-epoch detections are separated by 1.3" and 2.4 pix
The object was found in VSX13" Gaia DR3 4605967875067431296
Type: RS
# Max. Min./Amp. JD0 Period
16.590 G 16.730 G K
ATTENTION: measured mag 12.37 is 4.2 mag brighter than the VSX record maximum brightness 16.59 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:46.29 +36:31:17.3: 13.51 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:46.29 +36:31:17.3: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4605967875067431296,2461239.7595,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605967875067431296 20260718.2595 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.64 18:21:05.80 +36:03:22.3
63.59759 21.30658 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2741+36.0562 | 18:21:05.80 +36:03:22.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:05.80 +36:03:22.3: 12.80 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:05.80 +36:03:22.3: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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
ATO J275.2741+36.0562,2461239.7595,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.2741+36.0562 20260718.2595 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.30 18:20:35.26 +35:55:01.5
63.42065 21.35937 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605702274289792640 | 18:20:35.27 +35:55:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.448+/-0.026 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:35.26 +35:55:01.5: 12.28 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:35.26 +35:55:01.5: 12.26 +/- 0.01 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
Gaia DR3 4605702274289792640,2461239.7595,11.30,0.05,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
Gaia DR3 4605702274289792640 20260718.2595 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.72 18:20:52.29 +35:01:34.3
62.53689 21.01581 galactic Lyr Second-epoch detections are separated by 2.6" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:52.29 +35:01:34.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.325+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:52.29 +35:01:34.3: 13.97 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:52.29 +35:01:34.3: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
target,2461239.7595,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.64 18:20:09.14 +35:07:53.0
62.59203 21.18922 galactic Lyr Second-epoch detections are separated by 1.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:09.14 +35:07:53.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.402+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:09.14 +35:07:53.0: 13.94 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:09.14 +35:07:53.0: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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
target,2461239.7595,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.39 18:20:15.86 +35:43:55.0
63.20978 21.36191 galactic Lyr Second-epoch detections are separated by 4.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:15.86 +35:43:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:15.86 +35:43:55.0: 13.51 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:15.86 +35:43:55.0: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461239.7595,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.14 18:20:59.23 +36:09:09.9
63.68814 21.35852 galactic Lyr Second-epoch detections are separated by 0.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2550+36.1467 | 18:20:59.24 +36:09:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:59.23 +36:09:09.9: 12.26 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:59.23 +36:09:09.9: 12.18 +/- 0.01 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
ATO J275.2550+36.1467,2461239.7595,11.14,0.05,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 J275.2550+36.1467 20260718.2595 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.23 18:18:16.25 +36:31:49.8
63.88728 21.99700 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:16.25 +36:31:49.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.287+/-0.032 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:16.25 +36:31:49.8: 13.51 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:16.25 +36:31:49.8: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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
target,2461239.7595,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.41 18:26:34.05 +36:52:02.1
64.80107 20.52941 galactic Lyr Second-epoch detections are separated by 0.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:34.05 +36:52:02.1 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:34.05 +36:52:02.1: 13.51 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:34.05 +36:52:02.1: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.93 18:26:09.35 +36:30:32.5
64.41089 20.48972 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2095817326032624512 | 18:26:07.81 +36:30:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:09.35 +36:30:32.5: 12.79 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:09.35 +36:30:32.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 2095817326032624512,2461239.7595,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2095817326032624512 20260718.2595 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.91 18:21:24.59 +35:06:19.7
62.65576 20.93770 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:24.59 +35:06:19.7 (user input) | T | P | (position from user input) J-Ks=0.552+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:24.59 +35:06:19.7: 13.20 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:24.59 +35:06:19.7: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 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,2461239.7595,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.16 18:26:19.58 +36:40:05.0
64.58324 20.50967 galactic Lyr Second-epoch detections are separated by 2.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.5772+36.6620 | 18:26:19.58 +36:40:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.427+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:19.58 +36:40:05.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:19.58 +36:40:05.0: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.5772+36.6620,2461239.7595,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.5772+36.6620 20260718.2595 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.37 18:21:38.96 +35:14:57.1
62.81831 20.93855 galactic Lyr Second-epoch detections are separated by 0.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.4067+35.2489 | 18:21:38.95 +35:14:56.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.511+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:38.96 +35:14:57.1: 12.25 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:38.96 +35:14:57.1: 12.20 +/- 0.01 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
ATO J275.4067+35.2489,2461239.7595,11.37,0.05,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 J275.4067+35.2489 20260718.2595 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.49 18:19:35.89 +36:17:49.0
63.73905 21.67000 galactic Lyr Second-epoch detections are separated by 1.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:35.89 +36:17:49.0 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.037 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:35.89 +36:17:49.0: 13.74 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:35.89 +36:17:49.0: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.20 18:19:17.44 +35:16:42.8
62.68027 21.40341 galactic Lyr Second-epoch detections are separated by 1.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:17.44 +35:16:42.8 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:17.44 +35:16:42.8: 13.20 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:17.44 +35:16:42.8: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.02 18:18:25.71 +36:35:10.4
63.95504 21.98436 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.6084+36.5744 | 18:18:25.71 +36:35:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.678+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:25.71 +36:35:10.4: 13.20 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:25.71 +36:35:10.4: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.6084+36.5744,2461239.7595,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.6084+36.5744 20260718.2595 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.08 18:25:55.58 +37:02:24.6
64.93099 20.70695 galactic Lyr Second-epoch detections are separated by 0.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:55.58 +37:02:24.6 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:55.58 +37:02:24.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:55.58 +37:02:24.6: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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,2461239.7595,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.96 18:21:59.21 +36:04:36.7
63.68077 21.14295 galactic Lyr Second-epoch detections are separated by 1.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:59.21 +36:04:36.7 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:59.21 +36:04:36.7: 13.19 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:59.21 +36:04:36.7: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.91 18:17:43.21 +36:46:57.2
64.10866 22.18044 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:43.21 +36:46:57.2 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:43.21 +36:46:57.2: 13.21 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:43.21 +36:46:57.2: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.23 18:24:51.53 +36:33:42.8
64.37307 20.75319 galactic Lyr Second-epoch detections are separated by 1.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:24:51.53 +36:33:42.8 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.027 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:24:51.53 +36:33:42.8: 13.18 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:24:51.53 +36:33:42.8: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461239.7595,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.63 18:25:48.28 +36:48:27.2
64.68747 20.65411 galactic Lyr Second-epoch detections are separated by 1.7" and 2.5 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 J276.4560+36.7971 | 18:25:48.28 +36:48:27.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:48.28 +36:48:27.2: 14.14 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:48.28 +36:48:27.2: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 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 J276.4560+36.7971,2461239.7595,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.4560+36.7971 20260718.2595 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.21 18:21:17.23 +35:50:46.1
63.39756 21.20238 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605699216273290880 | 18:21:17.22 +35:50:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.781+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:17.23 +35:50:46.1: 12.25 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:17.23 +35:50:46.1: 12.21 +/- 0.01 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 4605699216273290880,2461239.7595,11.21,0.05,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 4605699216273290880 20260718.2595 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.65 18:17:55.89 +36:38:09.6
63.97248 22.09464 galactic Lyr Second-epoch detections are separated by 2.9" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.4907+36.6407 | 18:17:55.89 +36:38:09.6 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.398+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:55.89 +36:38:09.6: 14.14 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:55.89 +36:38:09.6: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 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 J274.4907+36.6407,2461239.7595,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.4907+36.6407 20260718.2595 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.94 18:16:39.70 +36:56:22.8
64.19962 22.43030 galactic Lyr Second-epoch detections are separated by 2.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.1585+36.9489 | 18:16:39.70 +36:56:22.8 (user input) | SINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.369+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:39.70 +36:56:22.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:39.70 +36:56:22.8: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 J274.1585+36.9489,2461239.7595,11.94,0.05,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
ATO J274.1585+36.9489 20260718.2595 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.23 18:20:09.53 +35:45:59.8
63.23764 21.39332 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:09.53 +35:45:59.8 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.612+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:09.53 +35:45:59.8: 13.48 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:09.53 +35:45:59.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 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
target,2461239.7595,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.57 18:19:33.35 +35:23:16.9
62.81030 21.38753 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:33.35 +35:23:16.9 (user input) | T | P | (position from user input) J-Ks=0.237+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:33.35 +35:23:16.9: 13.49 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:33.35 +35:23:16.9: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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
target,2461239.7595,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.37 18:21:06.66 +36:16:57.2
63.82877 21.37645 galactic Lyr Second-epoch detections are separated by 1.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:06.66 +36:16:57.2 (user input) | T | P | (position from user input) J-Ks=0.555+/-0.033 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:06.66 +36:16:57.2: 13.49 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:06.66 +36:16:57.2: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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
target,2461239.7595,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.15 18:20:52.60 +35:09:51.5
62.67711 21.05995 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2228+35.1642 | 18:20:52.60 +35:09:51.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.273+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:52.60 +35:09:51.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:52.60 +35:09:51.5: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.2228+35.1642,2461239.7595,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.2228+35.1642 20260718.2595 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.56 18:20:42.19 +36:10:54.9
63.69810 21.42216 galactic Lyr Second-epoch detections are separated by 1.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2107759499778738816 | 18:20:44.27 +36:10:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.444+/-0.031 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:42.19 +36:10:54.9: 13.72 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:42.19 +36:10:54.9: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 2107759499778738816,2461239.7595,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2107759499778738816 20260718.2595 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.47 18:27:36.25 +36:59:42.3
65.00257 20.37573 galactic Lyr Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.8991+36.9980 | 18:27:36.25 +36:59:42.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.382+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:36.25 +36:59:42.3: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:36.25 +36:59:42.3: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.8991+36.9980,2461239.7595,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.8991+36.9980 20260718.2595 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.52 18:17:33.87 +36:42:58.2
64.03005 22.18950 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:33.87 +36:42:58.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.368+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:33.87 +36:42:58.2: 12.78 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:33.87 +36:42:58.2: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 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
target,2461239.7595,11.52,0.05,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 20260718.2595 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 07 18.2595 2461239.7595 11.77 18:20:16.18 +34:59:55.1
62.46584 21.12328 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:16.18 +34:59:55.1 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:16.18 +34:59:55.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:16.18 +34:59:55.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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
target,2461239.7595,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.85 18:23:51.35 +35:49:26.9
63.55689 20.70300 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:23:51.35 +35:49:26.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.198+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:51.35 +35:49:26.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:23:51.35 +35:49:26.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 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
target,2461239.7595,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.10 18:21:53.41 +35:11:15.3
62.77327 20.87188 galactic Lyr Second-epoch detections are separated by 0.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:53.41 +35:11:15.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.276+/-0.033 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:53.41 +35:11:15.3: 13.16 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:53.41 +35:11:15.3: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:20:25.31 +35:10:55.1
62.66254 21.15358 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:25.31 +35:10:55.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.295+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:25.31 +35:10:55.1: 13.49 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:25.31 +35:10:55.1: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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
target,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.23 18:19:46.79 +35:11:40.0
62.62950 21.28169 galactic Lyr Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:46.79 +35:11:40.0 (user input) | T | P | (position from user input) J-Ks=0.721+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:46.79 +35:11:40.0: 13.48 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:46.79 +35:11:40.0: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
target,2461239.7595,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.70 18:20:17.88 +35:17:23.6
62.76319 21.21257 galactic Lyr Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:17.88 +35:17:23.6 (user input) | T | P | (position from user input) J-Ks=0.569+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:17.88 +35:17:23.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:17.88 +35:17:23.6: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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
target,2461239.7595,11.70,0.05,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
target 20260718.2595 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 07 18.2595 2461239.7595 12.21 18:22:06.95 +35:10:40.0
62.77957 20.82511 galactic Lyr Second-epoch detections are separated by 0.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:06.95 +35:10:40.0 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:06.95 +35:10:40.0: 13.14 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:06.95 +35:10:40.0: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.27 18:20:11.40 +35:17:12.1
62.75227 21.23238 galactic Lyr Second-epoch detections are separated by 2.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0474+35.2865 | 18:20:11.40 +35:17:12.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.477+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:11.40 +35:17:12.1: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:11.40 +35:17:12.1: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 J275.0474+35.2865,2461239.7595,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0474+35.2865 20260718.2595 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.01 18:20:32.04 +35:15:23.7
62.74619 21.15619 galactic Lyr Second-epoch detections are separated by 1.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:32.04 +35:15:23.7 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:32.04 +35:15:23.7: 13.16 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:32.04 +35:15:23.7: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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,2461239.7595,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.32 18:22:04.90 +34:57:58.9
62.56358 20.76208 galactic Lyr Second-epoch detections are separated by 1.9" and 2.3 pix
The object was found in VSX 0" ZTF J182204.89+345758.9
Type: BY
# Max. Min./Amp. JD0 Period
13.613 g Y 0.082 g 2458232.99740 1.591066800000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:04.90 +34:57:58.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:04.90 +34:57:58.9: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J182204.89+345758.9,2461239.7595,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J182204.89+345758.9 20260718.2595 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.27 18:27:15.54 +36:12:12.6
64.18183 20.17899 galactic Lyr Second-epoch detections are separated by 1.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:15.54 +36:12:12.6 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.027 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:15.54 +36:12:12.6: 13.14 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:15.54 +36:12:12.6: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 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,2461239.7595,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.99 18:20:09.66 +35:02:50.1
62.50733 21.16015 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.0497+35.0566 | 18:20:09.66 +35:02:50.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.545+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:09.66 +35:02:50.1: 13.15 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:09.66 +35:02:50.1: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 J275.0497+35.0566,2461239.7595,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.0497+35.0566 20260718.2595 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.19 18:19:28.59 +35:57:54.6
63.39225 21.58784 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.8705+35.9618 | 18:19:28.59 +35:57:54.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.668+/-0.031 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:28.59 +35:57:54.6: 13.16 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:28.59 +35:57:54.6: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 J274.8705+35.9618,2461239.7595,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.8705+35.9618 20260718.2595 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.03 18:18:00.07 +36:50:12.1
64.18307 22.14376 galactic Lyr Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:00.07 +36:50:12.1 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:00.07 +36:50:12.1: 13.13 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:00.07 +36:50:12.1: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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,2461239.7595,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.79 18:19:32.80 +35:06:08.5
62.51943 21.29693 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.8867+35.1025 | 18:19:32.80 +35:06:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.558+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:32.80 +35:06:08.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:32.80 +35:06:08.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 J274.8867+35.1025,2461239.7595,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.8867+35.1025 20260718.2595 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.90 18:25:29.17 +36:32:12.6
64.39177 20.62593 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:29.17 +36:32:12.6 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.027 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:29.17 +36:32:12.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:29.17 +36:32:12.6: 12.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.76 +/- 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
target,2461239.7595,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.22 18:20:33.60 +35:43:43.7
63.22734 21.30409 galactic Lyr Second-epoch detections are separated by 0.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.1383+35.7267 | 18:20:33.62 +35:43:44.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.521+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:33.60 +35:43:43.7: 12.18 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:33.60 +35:43:43.7: 12.18 +/- 0.01 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 J275.1383+35.7267,2461239.7595,11.22,0.05,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
ATO J275.1383+35.7267 20260718.2595 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.21 18:20:43.68 +35:44:26.9
63.25133 21.27569 galactic Lyr Second-epoch detections are separated by 0.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605691343594614400 | 18:20:43.66 +35:44:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:43.68 +35:44:26.9: 12.17 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:43.68 +35:44:26.9: 12.14 +/- 0.01 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
Gaia DR3 4605691343594614400,2461239.7595,11.21,0.05,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 4605691343594614400 20260718.2595 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.20 18:18:12.38 +36:32:10.8
63.88888 22.01113 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605978694091677312 | 18:18:12.11 +36:32:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:12.38 +36:32:10.8: 12.18 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:12.38 +36:32:10.8: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 4605978694091677312,2461239.7595,11.20,0.05,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
Gaia DR3 4605978694091677312 20260718.2595 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.10 18:20:32.77 +35:25:08.5
62.91182 21.20659 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:32.77 +35:25:08.5 (user input) | T | P | (position from user input) J-Ks=0.675+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:32.77 +35:25:08.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:32.77 +35:25:08.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.30 18:21:31.45 +36:04:17.8
63.64309 21.22974 galactic Lyr Second-epoch detections are separated by 0.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:31.45 +36:04:17.8 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.970+/-0.030 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:31.45 +36:04:17.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:31.45 +36:04:17.8: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.55 18:20:01.26 +35:18:18.1
62.75889 21.27094 galactic Lyr Second-epoch detections are separated by 1.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:01.26 +35:18:18.1 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:01.26 +35:18:18.1: 13.69 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:01.26 +35:18:18.1: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.56 18:17:11.95 +37:10:04.0
64.47005 22.39817 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was found in VSX 5" ZTF J181712.40+371003.8
Type: BY
# Max. Min./Amp. JD0 Period
16.551 g Y 0.070 g 2458204.98290 0.287542300000
ATTENTION: measured mag 12.56 is 3.9 mag brighter than the VSX record maximum brightness 16.48 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:11.95 +37:10:04.0: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:11.95 +37:10:04.0: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
ZTF J181712.40+371003.8,2461239.7595,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J181712.40+371003.8 20260718.2595 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.19 18:20:07.78 +35:03:31.2
62.51667 21.16993 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593626922197786112 | 18:20:07.79 +35:03:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:07.78 +35:03:31.2: 12.16 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:07.78 +35:03:31.2: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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 4593626922197786112,2461239.7595,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4593626922197786112 20260718.2595 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.73 18:19:23.12 +35:14:06.5
62.64284 21.37110 galactic Lyr Second-epoch detections are separated by 1.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:23.12 +35:14:06.5 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.035 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:23.12 +35:14:06.5: 13.94 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:23.12 +35:14:06.5: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.65 18:20:55.53 +35:57:41.0
63.48929 21.30887 galactic Lyr Second-epoch detections are separated by 0.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:55.53 +35:57:41.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.400+/-0.035 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:55.53 +35:57:41.0: 14.37 +/- 0.07 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:55.53 +35:57:41.0: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.16 +/- 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
target,2461239.7595,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.52 18:19:21.78 +35:46:52.2
63.19686 21.55089 galactic Lyr Second-epoch detections are separated by 3.1" and 2.4 pix
The object was found in VSX17" CSS_J181923.0+354648
Type: EB
# Max. Min./Amp. JD0 Period
16.510 CV Y 0.430 CV 3.714100000000
ATTENTION: measured mag 12.52 is 3.6 mag brighter than the VSX record maximum brightness 16.08 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:21.78 +35:46:52.2: 13.46 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:21.78 +35:46:52.2: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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
CSS_J181923.0+354648,2461239.7595,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J181923.0+354648 20260718.2595 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.91 18:21:02.95 +35:55:38.0
63.46322 21.27417 galactic Lyr Second-epoch detections are separated by 1.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:02.95 +35:55:38.0 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:02.95 +35:55:38.0: 13.09 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:02.95 +35:55:38.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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,2461239.7595,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.07 18:16:29.88 +37:00:31.6
64.25996 22.48259 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:29.88 +37:00:31.6 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:29.88 +37:00:31.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:29.88 +37:00:31.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.12 18:22:06.38 +35:07:35.9
62.72722 20.81012 galactic Lyr Second-epoch detections are separated by 2.5" and 2.5 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 J275.5267+35.1293 | 18:22:10.13 +35:07:41.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.542+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:06.38 +35:07:35.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:06.38 +35:07:35.9: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 J275.5267+35.1293,2461239.7595,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.5267+35.1293 20260718.2595 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.98 18:20:19.67 +35:53:11.7
63.37148 21.39941 galactic Lyr Second-epoch detections are separated by 0.6" and 2.3 pix
The object was found in VSX 0" Gaia DR3 4605748728656068736
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.870 G 12.900 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:19.67 +35:53:11.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:19.67 +35:53:11.7: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 4605748728656068736,2461239.7595,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605748728656068736 20260718.2595 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.63 18:17:51.07 +36:40:45.5
64.01149 22.12343 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:51.07 +36:40:45.5 (user input) | T | P | (position from user input) J-Ks=0.631+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:51.07 +36:40:45.5: 13.92 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:51.07 +36:40:45.5: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461239.7595,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.58 18:20:52.79 +35:56:37.0
63.46803 21.31190 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:52.79 +35:56:37.0 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.035 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:52.79 +35:56:37.0: 12.73 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:52.79 +35:56:37.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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
target,2461239.7595,11.58,0.05,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
target 20260718.2595 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 07 18.2595 2461239.7595 12.24 18:21:43.51 +34:53:21.6
62.46002 20.80565 galactic Lyr Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:43.51 +34:53:21.6 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.037 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:43.51 +34:53:21.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:43.51 +34:53:21.6: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.34 18:19:54.93 +36:25:00.8
63.88324 21.64742 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:54.93 +36:25:00.8 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:54.93 +36:25:00.8: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:54.93 +36:25:00.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.73 18:20:09.35 +36:20:02.1
63.81512 21.57521 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:09.35 +36:20:02.1 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.027 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:09.35 +36:20:02.1: 12.74 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:09.35 +36:20:02.1: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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
target,2461239.7595,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.79 18:19:43.46 +36:00:36.9
63.45539 21.55470 galactic Lyr Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9329+36.0141 | 18:19:43.46 +36:00:36.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.283+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:43.46 +36:00:36.9: 12.74 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:43.46 +36:00:36.9: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 J274.9329+36.0141,2461239.7595,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9329+36.0141 20260718.2595 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.30 18:26:58.78 +36:47:15.0
64.74959 20.42531 galactic Lyr Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:58.78 +36:47:15.0 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:58.78 +36:47:15.0: 13.44 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:58.78 +36:47:15.0: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 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
target,2461239.7595,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.69 18:18:39.82 +36:28:28.7
63.85675 21.90453 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605966015342714368 | 18:18:39.82 +36:28:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.496+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:39.82 +36:28:28.7: 12.70 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:39.82 +36:28:28.7: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 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
Gaia DR3 4605966015342714368,2461239.7595,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605966015342714368 20260718.2595 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.10 18:21:46.48 +35:02:24.0
62.61580 20.84569 galactic Lyr Second-epoch detections are separated by 0.7" and 2.3 pix
The object was found in VSX 0" Gaia DR3 4593617919946206592
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.940 G 12.970 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:46.48 +35:02:24.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:46.48 +35:02:24.0: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 4593617919946206592,2461239.7595,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4593617919946206592 20260718.2595 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.39 18:15:40.41 +37:06:14.1
64.30378 22.66826 galactic Lyr Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:15:40.41 +37:06:14.1 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:40.41 +37:06:14.1: 13.44 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:40.41 +37:06:14.1: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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
target,2461239.7595,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.32 18:17:07.83 +36:51:40.7
64.15016 22.31701 galactic Lyr Second-epoch detections are separated by 0.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4606036560184485760 | 18:17:07.83 +36:51:40.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.386+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:07.83 +36:51:40.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:07.83 +36:51:40.7: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 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
Large-amplitude variable Gaia DR2 4606036560184485760,2461239.7595,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4606036560184485760 20260718.2595 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.89 18:20:17.13 +35:56:40.0
63.42740 21.42609 galactic Lyr Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:17.13 +35:56:40.0 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:17.13 +35:56:40.0: 13.07 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:17.13 +35:56:40.0: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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
target,2461239.7595,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.38 18:16:28.59 +36:58:45.7
64.22823 22.47768 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:28.59 +36:58:45.7 (user input) | T | P | (position from user input) J-Ks=0.737+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:28.59 +36:58:45.7: 13.67 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:28.59 +36:58:45.7: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461239.7595,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.63 18:21:17.39 +35:03:52.7
62.60583 20.94751 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593628635886667008 | 18:21:18.88 +35:03:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.418+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:17.39 +35:03:52.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:17.39 +35:03:52.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 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
Gaia DR3 4593628635886667008,2461239.7595,11.63,0.05,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 4593628635886667008 20260718.2595 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.79 18:27:56.66 +36:23:24.0
64.41814 20.11094 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:56.66 +36:23:24.0 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:56.66 +36:23:24.0: 12.69 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:56.66 +36:23:24.0: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 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
target,2461239.7595,11.79,0.05,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 20260718.2595 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.01 18:19:36.53 +36:30:54.3
63.96251 21.73696 galactic Lyr Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9028+36.5179 | 18:19:36.53 +36:30:54.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.336+/-0.031 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:36.53 +36:30:54.3: 13.06 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:36.53 +36:30:54.3: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.9028+36.5179,2461239.7595,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9028+36.5179 20260718.2595 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.20 18:21:42.28 +35:45:08.3
63.33177 21.09190 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605685261920922496 | 18:21:42.26 +35:45:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.630+/-0.026 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:42.28 +35:45:08.3: 12.09 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:42.28 +35:45:08.3: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4605685261920922496,2461239.7595,11.20,0.05,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
Gaia DR3 4605685261920922496 20260718.2595 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.43 18:21:21.19 +35:18:41.3
62.86018 21.01603 galactic Lyr Second-epoch detections are separated by 2.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.3383+35.3068 | 18:21:21.19 +35:18:41.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.378+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:21.19 +35:18:41.3: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:21.19 +35:18:41.3: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 J275.3383+35.3068,2461239.7595,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.3383+35.3068 20260718.2595 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.08 18:26:13.77 +36:59:13.5
64.89844 20.63244 galactic Lyr Second-epoch detections are separated by 0.6" and 2.3 pix
The object was found in VSX 1" Gaia DR3 2107866255484880128
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.900 G 12.930 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:13.77 +36:59:13.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:13.77 +36:59:13.5: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 2107866255484880128,2461239.7595,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2107866255484880128 20260718.2595 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.06 18:20:44.26 +36:10:32.8
63.69424 21.41360 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2107759499778738816 | 18:20:44.27 +36:10:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:44.26 +36:10:32.8: 12.07 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:44.26 +36:10:32.8: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 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 2107759499778738816,2461239.7595,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2107759499778738816 20260718.2595 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.02 18:17:41.34 +36:48:19.6
64.13007 22.19347 galactic Lyr Second-epoch detections are separated by 1.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.4197+36.8027 | 18:17:41.34 +36:48:19.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:41.34 +36:48:19.6: 13.42 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:41.34 +36:48:19.6: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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
ATO J274.4197+36.8027,2461239.7595,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.4197+36.8027 20260718.2595 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.55 18:20:51.60 +35:06:31.8
62.61974 21.04506 galactic Lyr Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593632660274060672 | 18:20:51.58 +35:06:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.563+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:51.60 +35:06:31.8: 12.68 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:51.60 +35:06:31.8: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 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
Gaia DR3 4593632660274060672,2461239.7595,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4593632660274060672 20260718.2595 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.09 18:18:41.96 +36:39:05.2
64.04017 21.95314 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605981412804365440 | 18:18:41.97 +36:39:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:41.96 +36:39:05.2: 12.01 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:41.96 +36:39:05.2: 11.98 +/- 0.01 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
Gaia DR3 4605981412804365440,2461239.7595,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605981412804365440 20260718.2595 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.02 18:17:37.36 +36:37:17.3
63.93676 22.14901 galactic Lyr Second-epoch detections are separated by 0.2" and 2.1 pix
The object was found in VSX 1" HAT-P-5
Type: EP
# Max. Min./Amp. JD0 Period
12.030 V Y 0.014 V 2454241.77663 2.788491000000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:37.36 +36:37:17.3: 12.01 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:37.36 +36:37:17.3: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT-P-5,2461239.7595,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT-P-5 20260718.2595 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.96 18:20:27.60 +35:35:25.4
63.07969 21.27865 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:27.60 +35:35:25.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.301+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:27.60 +35:35:25.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:27.60 +35:35:25.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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
target,2461239.7595,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.79 18:21:02.14 +35:11:59.1
62.72438 21.04082 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:02.14 +35:11:59.1 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:02.14 +35:11:59.1: 13.04 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:02.14 +35:11:59.1: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.79,0.05,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 20260718.2595 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.12 18:21:54.62 +34:51:53.7
62.44877 20.76175 galactic Lyr Second-epoch detections are separated by 2.1" and 2.0 pix
The object was found in VSX 1" CSS_J182154.6+345153
Type: RRC
# Max. Min./Amp. JD0 Period
13.040 CV Y 0.220 CV 0.373676000000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:54.62 +34:51:53.7: 13.04 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:54.62 +34:51:53.7: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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
CSS_J182154.6+345153,2461239.7595,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J182154.6+345153 20260718.2595 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.10 18:19:55.32 +35:15:00.1
62.69603 21.27224 galactic Lyr Second-epoch detections are separated by 0.5" and 2.3 pix
The object was found in VSX 4" Gaia DR3 4605641899932839808
Type: ROT
# Max. Min./Amp. JD0 Period
14.910 G 14.940 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:55.32 +35:15:00.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:55.32 +35:15:00.1: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 4605641899932839808,2461239.7595,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605641899932839808 20260718.2595 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.88 18:20:49.28 +35:55:21.2
63.44254 21.31634 galactic Lyr Second-epoch detections are separated by 0.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2064+35.9210 | 18:20:49.28 +35:55:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:49.28 +35:55:21.2: 13.03 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:49.28 +35:55:21.2: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J275.2064+35.9210,2461239.7595,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.2064+35.9210 20260718.2595 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:19:30.30 +35:08:53.2
62.56292 21.31982 galactic Lyr Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:30.30 +35:08:53.2 (user input) | T | P | (position from user input) J-Ks=0.281+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:30.30 +35:08:53.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:30.30 +35:08:53.2: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 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
target,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.71 18:19:58.01 +35:58:15.6
63.43225 21.49568 galactic Lyr Second-epoch detections are separated by 1.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:58.01 +35:58:15.6 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:58.01 +35:58:15.6: 13.94 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:58.01 +35:58:15.6: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
target,2461239.7595,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.47 18:18:06.54 +36:35:11.0
63.93359 22.04533 galactic Lyr Second-epoch detections are separated by 1.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.5287+36.5841 | 18:18:08.18 +36:34:35.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:06.54 +36:35:11.0: 13.87 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:06.54 +36:35:11.0: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.5287+36.5841,2461239.7595,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.5287+36.5841 20260718.2595 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.07 18:17:11.10 +36:50:42.1
64.13705 22.30162 galactic Lyr Second-epoch detections are separated by 1.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:11.10 +36:50:42.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.382+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:11.10 +36:50:42.1: 13.45 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:11.10 +36:50:42.1: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
target,2461239.7595,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.20 18:20:07.81 +35:01:52.7
62.48896 21.16093 galactic Lyr Second-epoch detections are separated by 2.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:07.81 +35:01:52.7 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:07.81 +35:01:52.7: 13.43 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:07.81 +35:01:52.7: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.09 18:21:21.37 +36:11:25.2
63.75201 21.30005 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:21.37 +36:11:25.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.298+/-0.033 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:21.37 +36:11:25.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:21.37 +36:11:25.2: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 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
target,2461239.7595,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.43 18:19:38.31 +35:54:42.7
63.34918 21.53975 galactic Lyr Second-epoch detections are separated by 2.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.9166+35.9090 | 18:19:38.31 +35:54:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.615+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:38.31 +35:54:42.7: 13.41 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:38.31 +35:54:42.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
ATO J274.9166+35.9090,2461239.7595,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.9166+35.9090 20260718.2595 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.96 18:20:17.51 +35:46:15.0
63.25125 21.36913 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was found in VSX 1" Gaia DR3 4605694921305446912
Type: ROT
# Max. Min./Amp. JD0 Period
12.760 G 12.800 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:17.51 +35:46:15.0: 13.03 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:17.51 +35:46:15.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 4605694921305446912,2461239.7595,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605694921305446912 20260718.2595 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.03 18:19:52.56 +35:57:21.6
63.41066 21.50830 galactic Lyr Second-epoch detections are separated by 0.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:52.56 +35:57:21.6 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.031 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:52.56 +35:57:21.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:52.56 +35:57:21.6: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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,2461239.7595,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.04 18:27:19.20 +37:15:39.5
65.25079 20.51648 galactic Lyr Second-epoch detections are separated by 0.9" and 2.1 pix
The object was found in VSX 1" Gaia DR3 2107877246302701824
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.920 G 12.980 G A
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:19.20 +37:15:39.5: 13.01 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:19.20 +37:15:39.5: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 2107877246302701824,2461239.7595,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2107877246302701824 20260718.2595 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.24 18:20:19.40 +36:16:23.6
63.76480 21.52390 galactic Lyr Second-epoch detections are separated by 1.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:19.40 +36:16:23.6 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:19.40 +36:16:23.6: 13.39 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:19.40 +36:16:23.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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
target,2461239.7595,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.35 18:19:32.11 +36:12:43.4
63.64809 21.65513 galactic Lyr Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.8830+36.2098 | 18:19:32.11 +36:12:43.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.392+/-0.034 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:32.11 +36:12:43.4: 13.39 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:32.11 +36:12:43.4: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.8830+36.2098,2461239.7595,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.8830+36.2098 20260718.2595 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:21:20.47 +35:35:19.5
63.14026 21.10863 galactic Lyr Second-epoch detections are separated by 2.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.3241+35.5929 | 18:21:20.47 +35:35:19.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:20.47 +35:35:19.5: 13.67 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:20.47 +35:35:19.5: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
ATO J275.3241+35.5929,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.3241+35.5929 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.39 18:26:49.82 +36:53:36.3
64.84587 20.48834 galactic Lyr Second-epoch detections are separated by 2.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:49.82 +36:53:36.3 (user input) | T | P | (position from user input) J-Ks=0.589+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:49.82 +36:53:36.3: 13.39 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:49.82 +36:53:36.3: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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
target,2461239.7595,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.40 18:18:45.52 +33:47:29.8
61.13435 21.02127 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:18:45.52 +33:47:29.8 (user input) | T | P | (position from user input) J-Ks=0.228+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:45.52 +33:47:29.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:45.52 +33:47:29.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.30 18:16:45.28 +36:56:58.9
64.21611 22.41569 galactic Lyr Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.1862+36.9516 | 18:16:45.28 +36:56:58.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.302+/-0.034 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:45.28 +36:56:58.9: 13.67 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:45.28 +36:56:58.9: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J274.1862+36.9516,2461239.7595,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.1862+36.9516 20260718.2595 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.49 18:15:59.65 +37:06:40.5
64.33241 22.60958 galactic Lyr Second-epoch detections are separated by 2.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.9983+37.1142 | 18:15:59.65 +37:06:40.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.503+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:59.65 +37:06:40.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:59.65 +37:06:40.5: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.9983+37.1142,2461239.7595,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.9983+37.1142 20260718.2595 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.55 18:17:17.50 +36:55:05.1
64.21928 22.30386 galactic Lyr Second-epoch detections are separated by 0.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:17.50 +36:55:05.1 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:17.50 +36:55:05.1: 14.12 +/- 0.07 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:17.50 +36:55:05.1: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
target,2461239.7595,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.75 18:19:45.92 +35:09:32.1
62.59240 21.27298 galactic Lyr Second-epoch detections are separated by 1.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:45.92 +35:09:32.1 (user input) | T | P | (position from user input) J-Ks=0.696+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:45.92 +35:09:32.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:45.92 +35:09:32.1: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 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
target,2461239.7595,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:20:45.35 +35:12:54.8
62.72007 21.09990 galactic Lyr Second-epoch detections are separated by 2.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:45.35 +35:12:54.8 (user input) | T | P | (position from user input) J-Ks=0.443+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:45.35 +35:12:54.8: 13.91 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:45.35 +35:12:54.8: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.83 18:20:48.12 +36:06:49.9
63.63571 21.38147 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was found in VSX24" Gaia DR3 4605752954904073344
Type: ROT
# Max. Min./Amp. JD0 Period
15.810 G 15.860 G K
ATTENTION: measured mag 11.83 is 4.0 mag brighter than the VSX record maximum brightness 15.81 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:48.12 +36:06:49.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:48.12 +36:06:49.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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
Gaia DR3 4605752954904073344,2461239.7595,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605752954904073344 20260718.2595 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.23 18:20:50.39 +35:53:03.5
63.40496 21.30048 galactic Lyr Second-epoch detections are separated by 1.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:50.39 +35:53:03.5 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:50.39 +35:53:03.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:50.39 +35:53:03.5: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461239.7595,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.59 18:17:22.82 +36:37:13.8
63.91946 22.19493 galactic Lyr Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606024499916098304 | 18:17:22.80 +36:37:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.026 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:22.82 +36:37:13.8: 12.65 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:22.82 +36:37:13.8: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 4606024499916098304,2461239.7595,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606024499916098304 20260718.2595 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.35 18:21:57.01 +35:59:21.1
63.58927 21.12162 galactic Lyr Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:57.01 +35:59:21.1 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.036 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:57.01 +35:59:21.1: 13.85 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:57.01 +35:59:21.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:23:52.95 +37:06:52.9
64.86550 21.11682 galactic Lyr Second-epoch detections are separated by 1.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.9681+37.1178 | 18:23:52.95 +37:06:52.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.421+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:52.95 +37:06:52.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:23:52.95 +37:06:52.9: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.9681+37.1178,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.9681+37.1178 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.10 18:26:33.88 +37:01:21.9
64.95780 20.58084 galactic Lyr Second-epoch detections are separated by 1.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:33.88 +37:01:21.9 (user input) | T | P | (position from user input) J-Ks=0.289+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:33.88 +37:01:21.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:33.88 +37:01:21.9: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.54 18:20:38.44 +35:53:23.9
63.39678 21.34050 galactic Lyr Second-epoch detections are separated by 1.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:38.44 +35:53:23.9 (user input) | T | P | (position from user input) J-Ks=0.609+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:38.44 +35:53:23.9: 13.63 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:38.44 +35:53:23.9: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461239.7595,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.55 18:22:17.46 +36:03:34.7
63.68462 21.07922 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2107705275813358464 | 18:22:17.46 +36:03:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.027 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:17.46 +36:03:34.7: 12.62 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:17.46 +36:03:34.7: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 2107705275813358464,2461239.7595,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2107705275813358464 20260718.2595 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.41 18:21:38.25 +35:00:00.4
62.56561 20.85909 galactic Lyr Second-epoch detections are separated by 1.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:38.25 +35:00:00.4 (user input) | T | P | (position from user input) J-Ks=0.285+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:38.25 +35:00:00.4: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:38.25 +35:00:00.4: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.55 18:21:41.25 +35:02:37.6
62.61334 20.86378 galactic Lyr Second-epoch detections are separated by 0.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:41.25 +35:02:37.6 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:41.25 +35:02:37.6: 13.63 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:41.25 +35:02:37.6: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461239.7595,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:20:41.77 +35:36:27.3
63.11380 21.23877 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:41.77 +35:36:27.3 (user input) | T | P | (position from user input) J-Ks=0.614+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:41.77 +35:36:27.3: 13.90 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:41.77 +35:36:27.3: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.51 18:15:48.38 +37:11:13.6
64.39839 22.66829 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:15:48.38 +37:11:13.6 (user input) | T | P | (position from user input) J-Ks=0.612+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:15:48.38 +37:11:13.6: 13.63 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:15:48.38 +37:11:13.6: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 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
target,2461239.7595,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.14 18:20:29.66 +35:41:56.9
63.19258 21.30714 galactic Lyr Second-epoch detections are separated by 1.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:29.66 +35:41:56.9 (user input) | T | P | (position from user input) J-Ks=0.870+/-0.029 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:29.66 +35:41:56.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:29.66 +35:41:56.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.90 18:17:18.34 +36:45:48.0
64.06115 22.25341 galactic Lyr Second-epoch detections are separated by 1.5" and 2.5 pix
The object was found in VSX 1" Gaia DR3 4606034773478075520
Type: ROT
# Max. Min./Amp. JD0 Period
14.290 G 14.320 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:18.34 +36:45:48.0: 14.54 +/- 0.08 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:18.34 +36:45:48.0: 14.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4606034773478075520,2461239.7595,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606034773478075520 20260718.2595 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:27:59.95 +36:49:13.0
64.85442 20.24349 galactic Lyr Second-epoch detections are separated by 2.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:59.95 +36:49:13.0 (user input) | T | P | (position from user input) J-Ks=0.684+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:59.95 +36:49:13.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:59.95 +36:49:13.0: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.65 18:16:32.23 +37:01:22.6
64.27715 22.47949 galactic Lyr Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606053873195994240 | 18:16:32.21 +37:01:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.351+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:32.23 +37:01:22.6: 12.61 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:32.23 +37:01:22.6: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 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
Gaia DR3 4606053873195994240,2461239.7595,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606053873195994240 20260718.2595 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.60 18:20:12.10 +36:02:51.4
63.52658 21.47518 galactic Lyr Second-epoch detections are separated by 0.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605753706519028736 | 18:20:12.10 +36:02:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:12.10 +36:02:51.4: 12.61 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:12.10 +36:02:51.4: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 4605753706519028736,2461239.7595,11.60,0.05,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 4605753706519028736 20260718.2595 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.90 18:21:05.85 +35:51:42.5
63.40016 21.24381 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605698048041943424 | 18:21:05.84 +35:51:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.966+/-0.030 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:05.85 +35:51:42.5: 11.84 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:05.85 +35:51:42.5: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 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
Gaia DR3 4605698048041943424,2461239.7595,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605698048041943424 20260718.2595 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.63 18:20:31.97 +35:43:18.5
63.21832 21.30705 galactic Lyr Second-epoch detections are separated by 0.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.1383+35.7267 | 18:20:33.62 +35:43:44.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.249+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:31.97 +35:43:18.5: 12.59 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:31.97 +35:43:18.5: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 J275.1383+35.7267,2461239.7595,11.63,0.05,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
ATO J275.1383+35.7267 20260718.2595 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.21 18:26:24.92 +37:11:09.6
65.11231 20.66225 galactic Lyr Second-epoch detections are separated by 1.7" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.5925+37.1838 | 18:26:24.92 +37:11:09.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.318+/-0.031 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:24.92 +37:11:09.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:24.92 +37:11:09.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.5925+37.1838,2461239.7595,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.5925+37.1838 20260718.2595 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.28 18:17:23.88 +36:37:51.5
63.93140 22.19481 galactic Lyr Second-epoch detections are separated by 2.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606024499916098304 | 18:17:22.80 +36:37:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.590+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:23.88 +36:37:51.5: 13.62 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:23.88 +36:37:51.5: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4606024499916098304,2461239.7595,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606024499916098304 20260718.2595 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.10 18:26:04.21 +37:03:38.3
64.96167 20.68648 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:04.21 +37:03:38.3 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:04.21 +37:03:38.3: 13.00 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:04.21 +37:03:38.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.48 18:20:45.14 +35:07:21.2
62.62593 21.07035 galactic Lyr Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.1980+35.1135 | 18:20:45.14 +35:07:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.879+/-0.027 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:45.14 +35:07:21.2: 13.89 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:45.14 +35:07:21.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.1980+35.1135,2461239.7595,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.1980+35.1135 20260718.2595 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.54 18:20:02.21 +36:07:33.7
63.59502 21.53177 galactic Lyr Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605755218347514752 | 18:20:02.23 +36:07:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:02.21 +36:07:33.7: 12.58 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:02.21 +36:07:33.7: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4605755218347514752,2461239.7595,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4605755218347514752 20260718.2595 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.29 18:28:14.94 +36:18:47.9
64.36298 20.02750 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:28:14.94 +36:18:47.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:28:14.94 +36:18:47.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:28:14.94 +36:18:47.9: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.71 18:19:51.15 +35:35:05.2
63.03124 21.39375 galactic Lyr Second-epoch detections are separated by 1.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:51.15 +35:35:05.2 (user input) | T | P | (position from user input) J-Ks=0.625+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:51.15 +35:35:05.2: 13.86 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:51.15 +35:35:05.2: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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
target,2461239.7595,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.16 18:16:55.14 +36:36:41.9
63.87936 22.28020 galactic Lyr Second-epoch detections are separated by 1.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:55.14 +36:36:41.9 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:55.14 +36:36:41.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:55.14 +36:36:41.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.36 18:21:38.73 +35:06:39.7
62.67830 20.89399 galactic Lyr Second-epoch detections are separated by 0.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593630392531266816 | 18:21:39.48 +35:06:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:38.73 +35:06:39.7: 13.64 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:38.73 +35:06:39.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4593630392531266816,2461239.7595,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4593630392531266816 20260718.2595 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.34 18:26:53.88 +36:55:50.0
64.88806 20.48775 galactic Lyr Second-epoch detections are separated by 1.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:53.88 +36:55:50.0 (user input) | T | P | (position from user input) J-Ks=0.615+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:53.88 +36:55:50.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:53.88 +36:55:50.0: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.37 18:26:35.10 +36:31:43.2
64.46099 20.41477 galactic Lyr Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.6398+36.5194 | 18:26:35.10 +36:31:43.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.745+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:35.10 +36:31:43.2: 13.31 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:35.10 +36:31:43.2: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.6398+36.5194,2461239.7595,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.6398+36.5194 20260718.2595 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.36 18:21:08.16 +36:00:06.7
63.54512 21.28157 galactic Lyr Second-epoch detections are separated by 2.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:08.16 +36:00:06.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:08.16 +36:00:06.7: 13.88 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:08.16 +36:00:06.7: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461239.7595,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.89 18:17:41.10 +36:50:46.7
64.17177 22.20688 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606036899485241856 | 18:17:41.08 +36:50:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.536+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:41.10 +36:50:46.7: 11.81 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:41.10 +36:50:46.7: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 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
Gaia DR3 4606036899485241856,2461239.7595,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606036899485241856 20260718.2595 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.62 18:17:10.84 +36:51:27.8
64.14982 22.30636 galactic Lyr Second-epoch detections are separated by 1.8" and 2.4 pix
The object was found in VSX 1" Gaia DR3 4606036658967073152
Type: ROT
# Max. Min./Amp. JD0 Period
13.830 G 13.850 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:10.84 +36:51:27.8: 14.06 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:10.84 +36:51:27.8: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 4606036658967073152,2461239.7595,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606036658967073152 20260718.2595 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.78 18:18:36.64 +36:34:56.4
63.96339 21.94841 galactic Lyr Second-epoch detections are separated by 0.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4605980034115967360 | 18:18:36.64 +36:34:56.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.377+/-0.039 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:36.64 +36:34:56.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:36.64 +36:34:56.4: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4605980034115967360,2461239.7595,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4605980034115967360 20260718.2595 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.03 18:26:15.52 +36:30:44.3
64.42145 20.47128 galactic Lyr Second-epoch detections are separated by 1.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:15.52 +36:30:44.3 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:15.52 +36:30:44.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:15.52 +36:30:44.3: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461239.7595,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.27 18:19:46.07 +36:07:22.6
63.57326 21.58228 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:46.07 +36:07:22.6 (user input) | T | P | (position from user input) J-Ks=0.261+/-0.033 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:46.07 +36:07:22.6: 13.31 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:46.07 +36:07:22.6: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.36 18:17:20.05 +36:46:50.9
64.08101 22.25339 galactic Lyr Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4606035357593630720 | 18:17:20.06 +36:46:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.298+/-0.027 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:20.05 +36:46:50.9: 12.52 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:20.05 +36:46:50.9: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 4606035357593630720,2461239.7595,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4606035357593630720 20260718.2595 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.52 18:27:29.01 +36:11:44.6
64.19010 20.13370 galactic Lyr Second-epoch detections are separated by 2.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:29.01 +36:11:44.6 (user input) | T | P | (position from user input) J-Ks=0.253+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:29.01 +36:11:44.6: 13.64 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:29.01 +36:11:44.6: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.12 18:20:17.29 +35:06:44.5
62.58243 21.15676 galactic Lyr Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:17.29 +35:06:44.5 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:17.29 +35:06:44.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:17.29 +35:06:44.5: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
target,2461239.7595,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.40 18:19:21.79 +35:31:11.9
62.93093 21.46715 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:21.79 +35:31:11.9 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:21.79 +35:31:11.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:21.79 +35:31:11.9: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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
target,2461239.7595,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.22 18:20:18.12 +36:21:07.3
63.84365 21.55306 galactic Lyr Second-epoch detections are separated by 3.1" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:18.12 +36:21:07.3 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:18.12 +36:21:07.3: 13.41 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:18.12 +36:21:07.3: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.22,0.05,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
target 20260718.2595 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.45 18:24:33.46 +37:22:21.6
65.17358 21.07227 galactic Lyr Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.1361+37.3700 | 18:24:33.46 +37:22:21.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.663+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:24:33.46 +37:22:21.6: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:24:33.46 +37:22:21.6: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.1361+37.3700,2461239.7595,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.1361+37.3700 20260718.2595 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.62 18:22:11.20 +35:39:36.5
63.27249 20.96940 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.5572+35.6601 | 18:22:11.17 +35:39:36.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.666+/-0.030 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:11.20 +35:39:36.5: 12.49 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:11.20 +35:39:36.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.5572+35.6601,2461239.7595,11.62,0.05,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 J275.5572+35.6601 20260718.2595 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.53 18:20:25.92 +36:19:43.6
63.82891 21.52084 galactic Lyr Second-epoch detections are separated by 1.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:25.92 +36:19:43.6 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:25.92 +36:19:43.6: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:25.92 +36:19:43.6: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461239.7595,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.72 18:17:01.30 +36:50:58.5
64.13085 22.33411 galactic Lyr Second-epoch detections are separated by 1.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:01.30 +36:50:58.5 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.033 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:17:01.30 +36:50:58.5: 14.26 +/- 0.07 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:17:01.30 +36:50:58.5: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.51 18:22:03.95 +35:47:58.2
63.40509 21.03794 galactic Lyr Second-epoch detections are separated by 0.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:03.95 +35:47:58.2 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:03.95 +35:47:58.2: 13.83 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:03.95 +35:47:58.2: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.81 18:20:58.03 +35:06:31.0
62.62719 21.02427 galactic Lyr Second-epoch detections are separated by 0.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593632625911252736 | 18:20:58.02 +35:06:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.817+/-0.027 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:58.03 +35:06:31.0: 11.72 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:58.03 +35:06:31.0: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 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
Gaia DR3 4593632625911252736,2461239.7595,10.81,0.05,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
Gaia DR3 4593632625911252736 20260718.2595 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.77 18:20:26.19 +35:05:09.8
62.56636 21.11950 galactic Lyr Second-epoch detections are separated by 0.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4593627300154898176 | 18:20:26.18 +35:05:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.942+/-0.035 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:26.19 +35:05:09.8: 11.71 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:26.19 +35:05:09.8: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 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
Gaia DR3 4593627300154898176,2461239.7595,10.77,0.05,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 4593627300154898176 20260718.2595 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 10.76 18:20:31.43 +36:08:32.3
63.64534 21.44379 galactic Lyr Second-epoch detections are separated by 0.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4605756115999997824 | 18:20:31.45 +36:08:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:31.43 +36:08:32.3: 11.69 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:31.43 +36:08:32.3: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 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
Gaia DR3 4605756115999997824,2461239.7595,10.76,0.05,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 4605756115999997824 20260718.2595 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.60 18:18:02.06 +36:54:14.0
64.25426 22.15829 galactic Lyr Second-epoch detections are separated by 0.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.5083+36.9038 | 18:18:02.01 +36:54:13.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.088+/-0.029 (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:18:02.06 +36:54:14.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:18:02.06 +36:54:14.0: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.5083+36.9038,2461239.7595,11.60,0.05,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 J274.5083+36.9038 20260718.2595 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.41 18:19:16.50 +35:22:55.7
62.78450 21.43982 galactic Lyr Second-epoch detections are separated by 0.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:16.50 +35:22:55.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.326+/-0.034 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:19:16.50 +35:22:55.7: 13.33 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:19:16.50 +35:22:55.7: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.99 18:22:53.10 +35:46:21.5
63.43587 20.87213 galactic Lyr Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:22:53.10 +35:46:21.5 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.030 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:53.10 +35:46:21.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:22:53.10 +35:46:21.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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
target,2461239.7595,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.53 18:23:10.68 +35:53:25.6
63.57578 20.85449 galactic Lyr Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2107693490422190208 | 18:23:10.67 +35:53:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.630+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:10.68 +35:53:25.6: 12.47 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:23:10.68 +35:53:25.6: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 2107693490422190208,2461239.7595,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2107693490422190208 20260718.2595 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.46 18:21:32.47 +35:05:01.3
62.64316 20.90518 galactic Lyr Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:32.47 +35:05:01.3 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.031 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:32.47 +35:05:01.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:32.47 +35:05:01.3: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.97 18:26:02.91 +36:30:46.2
64.40715 20.51134 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:02.91 +36:30:46.2 (user input) | T | P | (position from user input) J-Ks=0.794+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:26:02.91 +36:30:46.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:26:02.91 +36:30:46.2: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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
target,2461239.7595,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.46 18:20:43.45 +35:46:58.4
63.29381 21.29000 galactic Lyr Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:43.45 +35:46:58.4 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.038 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:43.45 +35:46:58.4: 12.47 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:43.45 +35:46:58.4: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 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
target,2461239.7595,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.88 18:20:09.86 +35:05:25.9
62.55145 21.17360 galactic Lyr Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:09.86 +35:05:25.9 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.378+/-0.030 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:09.86 +35:05:25.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:09.86 +35:05:25.9: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461239.7595,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.96 18:16:48.82 +37:09:26.1
64.43378 22.46807 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:16:48.82 +37:09:26.1 (user input) | T | P | (position from user input) J-Ks=0.239+/-0.032 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:48.82 +37:09:26.1: 12.96 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:16:48.82 +37:09:26.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.06 18:25:42.68 +39:17:45.6
67.20847 21.46537 galactic Lyr Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:42.68 +39:17:45.6 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.028 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:25:42.68 +39:17:45.6: 12.96 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:25:42.68 +39:17:45.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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
target,2461239.7595,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.31 18:14:43.24 +37:19:17.3
64.46661 22.91481 galactic Her Second-epoch detections are separated by 3.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:14:43.24 +37:19:17.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.627+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:14:43.24 +37:19:17.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:14:43.24 +37:19:17.3: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.2595* 18 14 43.24 +37 19 17.3 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.75 18:21:14.20 +35:06:38.9
62.64873 20.97291 galactic Lyr Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:14.20 +35:06:38.9 (user input) | T | P | (position from user input) J-Ks=1.020+/- (M)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:14.20 +35:06:38.9: 14.28 +/- 0.07 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:14.20 +35:06:38.9: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7595,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.99 18:27:26.25 +36:27:37.9
64.45287 20.23054 galactic Lyr Second-epoch detections are separated by 1.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:26.25 +36:27:37.9 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:26.25 +36:27:37.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:26.25 +36:27:37.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 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
target,2461239.7595,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.78 18:20:51.13 +35:53:57.9
63.42118 21.30298 galactic Lyr Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:51.13 +35:53:57.9 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.029 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:51.13 +35:53:57.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:51.13 +35:53:57.9: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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
target,2461239.7595,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.95 18:27:02.28 +36:32:23.1
64.50420 20.33254 galactic Lyr Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:02.28 +36:32:23.1 (user input) | T | P | (position from user input) J-Ks=0.307+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:27:02.28 +36:32:23.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:27:02.28 +36:32:23.1: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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
target,2461239.7595,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.85 18:20:56.60 +35:13:04.7
62.73624 21.06459 galactic Lyr Second-epoch detections are separated by 0.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J275.2309+35.2183 | 18:20:56.60 +35:13:04.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.632+/-0.029 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:56.60 +35:13:04.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:56.60 +35:13:04.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 J275.2309+35.2183,2461239.7595,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.2309+35.2183 20260718.2595 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 11.78 18:20:11.78 +36:12:01.9
63.68196 21.52501 galactic Lyr Second-epoch detections are separated by 1.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:11.78 +36:12:01.9 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.274+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:20:11.78 +36:12:01.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:20:11.78 +36:12:01.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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
target,2461239.7595,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2595 2461239.7595 12.63 18:21:09.78 +36:08:39.4
63.69175 21.32219 galactic Lyr Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:09.78 +36:08:39.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.315+/-0.034 (F)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:21:09.78 +36:08:39.4: 14.05 +/- 0.06 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-06-11_03-51-22_20.00sec_5.00C_LIGHT_0278.fits at 18:21:09.78 +36:08:39.4: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.04 +/- 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
target,2461239.7595,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2595 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
ERROR running VaST on the field Lyr-02-Q2b1x1 (wrong field? clouds? very bad focus?)
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
First image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Last image: 2461239.75968035 18.07.2026 06:13:46.382 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Lyr-02-Q2b1x1_015244_TTUQ2b1x1_2008450_VVGKEclE/fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 390
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.09
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: 92 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): 86833
Objects passed selection criteria: 86515
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 69914
Average stars matched: 57438.8 (82.1563 %)
Memory usage VmPeak: 2085868 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 08:45:10 CDT 2026
Host name: tau
############################################################
**** FOUND 18:31:02.72 +34:39:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216022_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216022_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
**** FOUND 18:19:59.37 +36:05:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216029_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216029_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216037_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216037_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216038_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216038_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216040_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216040_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216041_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216041_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216042_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216042_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216049_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216049_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
**** FOUND 18:35:15.24 +38:53:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216050_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216050_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216054_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216054_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216060_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216060_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216070_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216070_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 216073_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 216073_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 88473_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 88473_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
**** FOUND 18:36:56.67 +38:47:08.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 72022_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72022_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68218_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68218_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 17105_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 17105_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 68741_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68741_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62092_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62092_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 42327_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 42327_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40683_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40683_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72327_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 72327_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
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Considering the candidate 52769_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52769_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61475_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61475_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66002_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66002_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38725_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38725_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66357_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66357_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 85998_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 85998_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67507_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67507_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 101447_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 101447_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67079_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67079_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37857_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37857_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36411_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36411_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51729_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51729_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 54508_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 54508_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 58097_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 58097_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68992_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68992_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 79344_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 79344_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 70471_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 70471_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40731_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40731_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51979_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51979_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 79062_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 79062_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62909_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62909_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57209_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57209_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66170_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66170_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 76692_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 76692_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65424_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65424_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 79338_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 79338_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57694_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57694_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38960_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38960_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73035_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73035_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55470_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55470_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48281_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48281_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 78453_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 78453_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68421_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68421_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 59987_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 59987_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40142_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40142_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67338_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67338_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52852_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52852_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 45604_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 45604_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73438_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73438_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69116_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69116_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 75912_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 75912_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62242_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62242_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66745_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66745_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66028_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66028_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 79287_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 79287_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
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Considering the candidate 67193_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67193_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38310_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38310_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62241_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62241_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65110_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65110_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72594_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72594_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 78880_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 78880_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 35401_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 35401_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49740_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49740_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68769_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68769_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 42200_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 42200_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66013_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66013_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 77299_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 77299_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 21772_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 21772_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 71233_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 71233_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39739_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39739_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62004_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62004_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 56453_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 56453_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
**** FOUND 18:27:12.18 +36:14:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74800_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 74800_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61024_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61024_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73532_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73532_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73324_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73324_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53659_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53659_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73779_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73779_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73708_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73708_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40372_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40372_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66671_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66671_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61442_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61442_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 180847_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 180847_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 167121_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 167121_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63639_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63639_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 46633_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 46633_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48960_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48960_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63637_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63637_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 44158_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 44158_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67531_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67531_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49391_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49391_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52509_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52509_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65001_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65001_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51943_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51943_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68901_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68901_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 34590_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 34590_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37026_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37026_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49244_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49244_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73009_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73009_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69356_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69356_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 76118_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 76118_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 60738_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 60738_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49811_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49811_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55471_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55471_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40583_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40583_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 75281_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 75281_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51869_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51869_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 71462_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 71462_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61616_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61616_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36870_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36870_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 91124_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 91124_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55294_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55294_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39975_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39975_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69507_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69507_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36412_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36412_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37535_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37535_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49245_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49245_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 45800_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 45800_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 213484_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 213484_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 39350_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39350_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 50917_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 50917_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39547_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39547_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66966_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66966_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37436_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37436_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55823_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55823_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 76153_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 76153_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55870_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55870_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37320_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37320_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 76899_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 76899_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37934_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37934_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 56936_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 56936_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 78045_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 78045_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
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Considering the candidate 44053_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 44053_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 59462_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 59462_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57747_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57747_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 46310_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 46310_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 54405_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 54405_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51753_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51753_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 44584_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 44584_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 76427_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 76427_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
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Considering the candidate 58669_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 58669_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 71208_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 71208_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 60546_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 60546_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62748_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62748_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39972_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39972_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 76032_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 76032_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48638_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48638_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38142_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38142_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57300_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57300_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55424_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55424_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 45787_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 45787_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72349_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72349_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37901_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37901_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 46407_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 46407_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49362_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49362_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36553_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36553_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39342_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39342_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61776_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61776_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53812_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53812_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51617_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51617_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36740_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36740_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38541_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38541_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 200095_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 200095_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 48463_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48463_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55709_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55709_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62005_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62005_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66872_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66872_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61121_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61121_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38060_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38060_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63532_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63532_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 178910_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 178910_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 40486_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40486_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57917_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57917_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 41109_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 41109_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62917_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62917_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69890_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69890_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53925_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53925_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66280_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66280_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62036_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62036_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65843_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65843_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 50289_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 50289_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63736_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63736_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69185_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69185_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48937_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48937_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 42832_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 42832_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57564_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57564_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 185148_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 185148_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 39019_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39019_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55894_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55894_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69088_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69088_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65239_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65239_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36550_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36550_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49630_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49630_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39384_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39384_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39351_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39351_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39609_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39609_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 41250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 41250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39340_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39340_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 41056_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 41056_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40579_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40579_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 35767_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 35767_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 212072_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 212072_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 55787_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55787_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37277_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37277_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52467_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52467_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38204_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38204_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61457_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61457_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48523_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48523_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48637_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48637_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62229_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62229_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 43371_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 43371_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53900_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53900_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 41397_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 41397_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72993_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72993_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67145_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 67145_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
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Considering the candidate 37593_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37593_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40250_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52133_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52133_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49361_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49361_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51682_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51682_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 184474_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 184474_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 70341_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 70341_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38337_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38337_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51035_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51035_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 64524_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 64524_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52007_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52007_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 34478_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 34478_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 60114_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 60114_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 58701_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 58701_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53253_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53253_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65554_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65554_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61088_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61088_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37004_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37004_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72212_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72212_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67668_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67668_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52017_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52017_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69902_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69902_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37510_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37510_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 58938_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 58938_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61635_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61635_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48815_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48815_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 197563_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 197563_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 197457_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 197457_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 41374_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 41374_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69083_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69083_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55982_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55982_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66647_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66647_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38229_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38229_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 64216_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 64216_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63827_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63827_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 46075_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 46075_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39676_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39676_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 34038_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 34038_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 40602_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 40602_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51690_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51690_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38884_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38884_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52437_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52437_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62951_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62951_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67460_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67460_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37027_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37027_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 56052_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 56052_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51562_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51562_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49080_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49080_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52231_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52231_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73512_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73512_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57592_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57592_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 56572_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 56572_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 45892_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 45892_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67310_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67310_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 17278_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 17278_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69284_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69284_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72226_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72226_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68625_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68625_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38970_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38970_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39830_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39830_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 54833_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 54833_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 50863_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 50863_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63683_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63683_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52518_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52518_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 71398_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 71398_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 69542_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 69542_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 50987_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 50987_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53837_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53837_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 36296_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 36296_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37080_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37080_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 46285_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 46285_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 73442_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 73442_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 47770_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 47770_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65966_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 65966_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66061_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66061_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 70654_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 70654_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 53730_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 53730_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 50894_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 50894_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48232_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48232_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72430_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72430_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63792_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63792_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 70223_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 70223_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38397_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38397_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55082_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55082_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 57626_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 57626_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 45982_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 45982_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 63707_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 63707_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38117_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38117_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67961_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67961_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61198_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61198_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 52934_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 52934_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67686_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67686_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67624_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67624_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 62882_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 62882_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61142_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61142_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55065_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55065_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 66452_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 66452_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55655_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55655_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38205_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38205_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 44977_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 44977_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 58792_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 58792_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 75355_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 75355_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 47117_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 47117_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 58462_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 58462_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 67546_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 67546_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49302_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49302_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38367_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38367_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38055_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38055_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55520_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55520_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 68451_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 68451_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 71078_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 71078_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
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Considering the candidate 42770_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 42770_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 48844_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 48844_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 50905_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 50905_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 37657_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 37657_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61057_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61057_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 49222_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 49222_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 38017_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38017_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 72911_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 72911_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 105243_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 105243_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 75551_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 75551_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 74705_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 74705_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
**** FOUND 18:44:46.21 +37:36:19.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 38045_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 38045_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 65952_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
The candidate 65952_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225 did not pass the final checks
**** FOUND 18:54:30.06 +36:53:55.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 60080_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 60080_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 51196_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 51196_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 61437_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 61437_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 39922_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 39922_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 56315_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 56315_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
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Considering the candidate 55213_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
Preparing report for the candidate 55213_fd_Lyr-02-Q2b1x1_2026-07-18_01-13-46_20.00sec_4.90C_LIGHT_0225
make_report_in_HTML.sh Phase 2 (HTML assembly): 31s
make_report_in_HTML.sh TOTAL: 659s
Prepared the HTML report for the field Lyr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:32:54.76 +39:03:22.7
18:25:42.68 +39:17:45.6
18:20:55.56 +35:10:33.8
18:18:45.52 +33:47:29.8
18:19:27.19 +34:05:16.3
18:21:54.62 +34:51:53.7
18:21:43.51 +34:53:21.6
18:22:21.77 +34:54:00.4
18:21:54.73 +34:56:11.3
18:22:04.90 +34:57:58.9
18:21:38.25 +35:00:00.4
18:20:25.35 +34:59:41.3
18:20:44.69 +34:59:48.5
18:20:16.18 +34:59:55.1
18:21:20.68 +35:00:44.7
18:20:52.29 +35:01:34.3
18:20:15.59 +35:01:33.2
18:21:46.48 +35:02:24.0
18:19:30.44 +35:01:38.3
18:20:07.81 +35:01:52.7
18:21:41.25 +35:02:37.6
18:20:09.66 +35:02:50.1
18:19:56.00 +35:03:14.1
18:21:18.87 +35:03:38.1
18:21:17.39 +35:03:52.7
18:20:12.76 +35:03:37.0
18:20:07.78 +35:03:31.2
18:21:32.47 +35:05:01.3
18:21:06.43 +35:05:07.3
18:20:08.23 +35:05:07.3
18:19:37.36 +35:05:18.7
18:20:09.86 +35:05:25.9
18:21:14.20 +35:06:38.9
18:20:26.19 +35:05:09.8
18:21:24.59 +35:06:19.7
18:21:38.73 +35:06:39.7
18:19:39.70 +35:05:43.0
18:19:32.80 +35:06:08.5
18:20:17.29 +35:06:44.5
18:20:51.60 +35:06:31.8
18:21:58.83 +35:07:13.8
18:22:06.38 +35:07:35.9
18:20:58.03 +35:06:31.0
18:20:45.14 +35:07:21.2
18:20:09.14 +35:07:53.0
18:20:36.82 +35:07:35.9
18:19:30.30 +35:08:53.2
18:21:40.01 +35:09:46.6
18:19:45.92 +35:09:32.1
18:20:52.60 +35:09:51.5
18:22:06.95 +35:10:40.0
18:20:56.48 +35:10:45.4
18:20:16.40 +35:10:53.1
18:20:25.31 +35:10:55.1
18:21:53.41 +35:11:15.3
18:19:35.15 +35:11:24.0
18:19:46.79 +35:11:40.0
18:21:02.14 +35:11:59.1
18:19:48.94 +35:12:14.2
18:20:45.35 +35:12:54.8
18:20:56.60 +35:13:04.7
18:19:59.20 +35:12:34.7
18:22:02.51 +35:13:38.4
18:21:11.00 +35:13:38.5
18:19:23.12 +35:14:06.5
18:20:04.91 +35:14:38.9
18:21:38.96 +35:14:57.1
18:20:32.04 +35:15:23.7
18:20:19.59 +35:15:32.3
18:19:55.32 +35:15:00.1
18:19:18.84 +35:15:31.9
18:20:02.39 +35:15:47.5
18:20:11.40 +35:17:12.1
18:19:17.44 +35:16:42.8
18:20:17.88 +35:17:23.6
18:21:21.19 +35:18:41.3
18:20:01.26 +35:18:18.1
18:20:05.97 +35:20:47.7
18:21:38.39 +35:22:32.0
18:19:16.50 +35:22:55.7
18:19:33.35 +35:23:16.9
18:20:32.77 +35:25:08.5
18:21:44.02 +35:28:26.2
18:20:05.29 +35:28:00.2
18:22:28.47 +35:30:41.5
18:19:21.79 +35:31:11.9
18:22:44.76 +35:34:27.0
18:21:05.44 +35:34:18.6
18:20:02.08 +35:34:42.9
18:21:20.47 +35:35:19.5
18:19:51.15 +35:35:05.2
18:20:27.60 +35:35:25.4
18:20:41.77 +35:36:27.3
18:21:39.39 +35:36:42.5
18:20:10.13 +35:36:44.6
18:21:34.99 +35:37:40.3
18:22:11.20 +35:39:36.5
18:20:29.66 +35:41:56.9
18:20:31.97 +35:43:18.5
18:20:29.47 +35:43:37.3
18:20:48.09 +35:43:33.7
18:20:15.86 +35:43:55.0
18:20:33.60 +35:43:43.7
18:20:43.68 +35:44:26.9
18:22:11.65 +35:45:27.2
18:21:42.28 +35:45:08.3
18:22:53.10 +35:46:21.5
18:20:09.53 +35:45:59.8
18:20:55.76 +35:45:50.3
18:20:17.51 +35:46:15.0
18:20:43.45 +35:46:58.4
18:21:07.98 +35:46:37.9
18:20:55.49 +35:46:50.2
18:22:03.95 +35:47:58.2
18:19:21.78 +35:46:52.2
18:23:48.96 +35:48:39.9
18:22:28.74 +35:48:07.7
18:23:51.35 +35:49:26.9
18:20:33.25 +35:49:00.3
18:23:08.03 +35:49:54.8
18:21:17.23 +35:50:46.1
18:20:50.39 +35:53:03.5
18:21:05.85 +35:51:42.5
18:23:10.68 +35:53:25.6
18:19:58.80 +35:52:40.9
18:20:38.44 +35:53:23.9
18:20:19.67 +35:53:11.7
18:20:51.13 +35:53:57.9
18:19:38.31 +35:54:42.7
18:20:35.26 +35:55:01.5
18:21:02.95 +35:55:38.0
18:20:49.28 +35:55:21.2
18:20:54.04 +35:55:49.0
18:19:39.78 +35:55:12.1
18:22:56.36 +35:56:58.7
18:22:06.80 +35:57:17.6
18:19:59.42 +35:56:26.6
18:20:52.79 +35:56:37.0
18:20:17.13 +35:56:40.0
18:20:55.53 +35:57:41.0
18:19:52.56 +35:57:21.6
18:19:58.01 +35:58:15.6
18:19:28.59 +35:57:54.6
18:20:22.59 +35:58:12.7
18:21:57.01 +35:59:21.1
18:22:54.85 +36:00:21.0
18:22:17.09 +36:00:29.1
18:21:08.16 +36:00:06.7
18:19:43.46 +36:00:36.9
18:18:53.44 +36:02:17.5
18:20:12.10 +36:02:51.4
18:21:05.80 +36:03:22.3
18:22:17.46 +36:03:34.7
18:21:31.45 +36:04:17.8
18:21:59.21 +36:04:36.7
18:20:58.88 +36:05:50.3
18:20:47.00 +36:05:52.4
18:20:48.12 +36:06:49.9
18:19:46.07 +36:07:22.6
18:20:02.21 +36:07:33.7
18:21:09.78 +36:08:39.4
18:27:47.72 +36:09:51.1
18:20:28.81 +36:08:37.9
18:19:48.26 +36:08:50.6
18:20:24.01 +36:09:20.1
18:20:31.43 +36:08:32.3
18:27:29.01 +36:11:44.6
18:20:59.23 +36:09:09.9
18:27:15.54 +36:12:12.6
18:20:58.35 +36:10:37.0
18:20:35.38 +36:10:32.0
18:20:42.19 +36:10:54.9
18:20:44.26 +36:10:32.8
18:21:21.37 +36:11:25.2
18:20:11.78 +36:12:01.9
18:19:32.11 +36:12:43.4
18:19:57.45 +36:14:17.2
18:28:25.53 +36:15:34.4
18:28:12.22 +36:17:47.5
18:21:06.66 +36:16:57.2
18:20:19.40 +36:16:23.6
18:28:14.94 +36:18:47.9
18:20:36.57 +36:17:20.7
18:20:14.77 +36:17:13.4
18:19:35.89 +36:17:49.0
18:20:01.37 +36:18:36.7
18:20:25.92 +36:19:43.6
18:20:05.05 +36:20:11.6
18:20:09.35 +36:20:02.1
18:20:18.12 +36:21:07.3
18:27:56.66 +36:23:24.0
18:26:50.38 +36:25:27.4
18:20:23.73 +36:25:30.8
18:27:26.25 +36:27:37.9
18:19:54.93 +36:25:00.8
18:26:38.99 +36:29:21.1
18:18:43.97 +36:27:44.8
18:17:32.96 +36:28:15.7
18:26:02.91 +36:30:46.2
18:18:39.82 +36:28:28.7
18:26:09.35 +36:30:32.5
18:26:15.52 +36:30:44.3
18:26:35.10 +36:31:43.2
18:27:02.28 +36:32:23.1
18:19:11.28 +36:30:14.4
18:25:29.17 +36:32:12.6
18:18:59.79 +36:30:15.6
18:21:56.21 +36:31:39.2
18:19:36.53 +36:30:54.3
18:18:46.29 +36:31:17.3
18:26:40.54 +36:34:19.4
18:18:16.25 +36:31:49.8
18:24:51.53 +36:33:42.8
18:27:47.76 +36:34:36.4
18:18:12.38 +36:32:10.8
18:18:34.80 +36:32:53.2
18:19:03.60 +36:33:07.4
18:19:07.29 +36:34:37.9
18:18:36.64 +36:34:56.4
18:26:56.02 +36:37:39.4
18:18:25.71 +36:35:10.4
18:18:06.54 +36:35:11.0
18:26:19.58 +36:40:05.0
18:18:38.25 +36:37:42.2
18:18:16.08 +36:37:46.4
18:17:22.82 +36:37:13.8
18:16:55.14 +36:36:41.9
18:17:55.89 +36:38:09.6
18:17:23.88 +36:37:51.5
18:17:37.36 +36:37:17.3
18:18:41.96 +36:39:05.2
18:17:51.07 +36:40:45.5
18:17:17.24 +36:42:08.8
18:18:19.52 +36:42:13.7
18:17:33.87 +36:42:58.2
18:17:24.41 +36:43:56.8
18:26:58.78 +36:47:15.0
18:25:48.28 +36:48:27.2
18:17:18.34 +36:45:48.0
18:17:36.21 +36:45:23.8
18:17:57.78 +36:46:05.5
18:16:28.94 +36:44:54.8
18:27:59.95 +36:49:13.0
18:16:26.75 +36:45:38.6
18:17:43.21 +36:46:57.2
18:17:54.65 +36:47:19.7
18:17:20.05 +36:46:50.9
18:17:41.34 +36:48:19.6
18:17:33.42 +36:47:07.2
18:16:33.62 +36:47:32.1
18:26:34.05 +36:52:02.1
18:27:38.95 +36:52:32.1
18:26:45.08 +36:52:48.1
18:16:52.13 +36:49:12.6
18:18:00.07 +36:50:12.1
18:26:49.82 +36:53:36.3
18:17:17.28 +36:50:22.7
18:17:11.10 +36:50:42.1
18:16:47.46 +36:50:30.6
18:16:14.04 +36:50:13.6
18:17:01.30 +36:50:58.5
18:17:10.84 +36:51:27.8
18:17:07.83 +36:51:40.7
18:17:41.10 +36:50:46.7
18:26:53.88 +36:55:50.0
18:17:16.34 +36:53:47.6
18:26:36.99 +36:57:29.7
18:18:02.06 +36:54:14.0
18:17:17.50 +36:55:05.1
18:26:30.95 +36:58:23.7
18:16:45.02 +36:54:47.1
18:26:43.57 +36:59:14.0
18:26:09.97 +36:58:52.6
18:26:13.77 +36:59:13.5
18:27:36.25 +36:59:42.3
18:16:34.78 +36:56:15.8
18:16:39.70 +36:56:22.8
18:16:45.28 +36:56:58.9
18:16:57.91 +36:56:40.3
18:15:56.36 +36:57:03.1
18:26:33.88 +37:01:21.9
18:25:55.58 +37:02:24.6
18:16:28.59 +36:58:45.7
18:26:04.21 +37:03:38.3
18:16:29.88 +37:00:31.6
18:25:56.89 +37:04:27.0
18:16:32.23 +37:01:22.6
18:16:20.70 +37:03:22.8
18:16:54.48 +37:03:34.5
18:23:52.95 +37:06:52.9
18:26:55.22 +37:08:05.7
18:26:57.73 +37:09:48.1
18:15:40.41 +37:06:14.1
18:15:59.65 +37:06:40.5
18:16:38.63 +37:07:34.1
18:26:24.92 +37:11:09.6
18:16:35.00 +37:08:31.9
18:16:48.82 +37:09:26.1
18:17:11.95 +37:10:04.0
18:15:38.00 +37:10:50.0
18:24:06.76 +37:13:19.9
18:26:06.96 +37:14:57.3
18:28:25.39 +37:15:31.4
18:15:48.38 +37:11:13.6
18:27:19.20 +37:15:39.5
18:26:43.33 +37:15:35.8
18:15:48.09 +37:12:21.0
18:25:27.50 +37:16:23.3
18:15:07.75 +37:16:07.9
18:15:22.99 +37:18:15.1
18:24:33.46 +37:22:21.6
18:14:43.24 +37:19:17.3
18:25:36.73 +37:24:42.1
18:26:10.02 +37:25:31.9
18:26:25.54 +37:25:40.5
18:26:22.68 +37:25:58.6
18:14:15.76 +37:22:54.7
18:26:07.17 +37:28:48.5
18:26:48.51 +37:30:11.4
18:26:04.39 +37:34:52.4
18:25:41.48 +37:36:35.3
18:13:33.91 +37:31:28.1
18:38:07.84 +37:38:16.8
18:26:03.15 +37:37:41.7
18:13:41.80 +37:57:28.6
18:12:31.18 +38:16:08.6
########### Completed Lyr-02-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 ####
18:26:57.73 +37:09:48.1
18:17:16.34 +36:53:47.6
18:20:29.47 +35:43:37.3
18:26:30.95 +36:58:23.7
18:27:47.76 +36:34:36.4
18:21:38.39 +35:22:32.0
18:19:18.84 +35:15:31.9
18:22:54.85 +36:00:21.0
18:18:59.79 +36:30:15.6
18:17:36.21 +36:45:23.8
18:20:36.82 +35:07:35.9
18:17:54.65 +36:47:19.7
18:13:41.80 +37:57:28.6
18:16:47.46 +36:50:30.6
18:32:54.76 +39:03:22.7
18:26:45.08 +36:52:48.1
18:21:06.43 +35:05:07.3
18:20:25.35 +34:59:41.3
18:20:54.04 +35:55:49.0
18:20:47.00 +36:05:52.4
18:20:01.37 +36:18:36.7
18:26:09.97 +36:58:52.6
18:26:03.15 +37:37:41.7
18:25:56.89 +37:04:27.0
18:20:02.39 +35:15:47.5
18:19:59.42 +35:56:26.6
18:13:33.91 +37:31:28.1
18:26:56.02 +36:37:39.4
18:28:25.53 +36:15:34.4
18:16:26.75 +36:45:38.6
18:14:15.76 +37:22:54.7
18:17:24.41 +36:43:56.8
18:38:07.84 +37:38:16.8
18:20:36.57 +36:17:20.7
18:21:40.01 +35:09:46.6
18:24:06.76 +37:13:19.9
18:19:48.26 +36:08:50.6
18:20:48.09 +35:43:33.7
18:26:04.39 +37:34:52.4
18:26:36.99 +36:57:29.7
18:20:23.73 +36:25:30.8
18:21:11.00 +35:13:38.5
18:17:17.28 +36:50:22.7
18:22:17.09 +36:00:29.1
18:22:44.76 +35:34:27.0
18:28:25.39 +37:15:31.4
18:16:34.78 +36:56:15.8
18:25:36.73 +37:24:42.1
18:19:03.60 +36:33:07.4
18:16:33.62 +36:47:32.1
18:16:28.94 +36:44:54.8
18:16:52.13 +36:49:12.6
18:21:58.83 +35:07:13.8
18:18:34.80 +36:32:53.2
18:18:19.52 +36:42:13.7
18:16:35.00 +37:08:31.9
18:25:41.48 +37:36:35.3
18:21:54.73 +34:56:11.3
18:20:33.25 +35:49:00.3
18:16:45.02 +36:54:47.1
18:20:05.97 +35:20:47.7
18:17:57.78 +36:46:05.5
18:26:48.51 +37:30:11.4
18:19:27.19 +34:05:16.3
18:16:54.48 +37:03:34.5
18:19:48.94 +35:12:14.2
18:26:40.54 +36:34:19.4
18:15:07.75 +37:16:07.9
18:17:32.96 +36:28:15.7
18:26:43.33 +37:15:35.8
18:26:06.96 +37:14:57.3
18:18:53.44 +36:02:17.5
18:25:27.50 +37:16:23.3
18:15:48.09 +37:12:21.0
18:20:04.91 +35:14:38.9
18:17:33.42 +36:47:07.2
18:19:11.28 +36:30:14.4
18:20:55.56 +35:10:33.8
18:18:16.08 +36:37:46.4
18:21:34.99 +35:37:40.3
18:20:55.76 +35:45:50.3
18:18:38.25 +36:37:42.2
18:20:05.29 +35:28:00.2
18:16:14.04 +36:50:13.6
18:22:28.74 +35:48:07.7
18:20:22.59 +35:58:12.7
18:17:17.24 +36:42:08.8
18:22:06.80 +35:57:17.6
18:26:43.57 +36:59:14.0
18:22:21.77 +34:54:00.4
18:19:30.44 +35:01:38.3
18:21:07.98 +35:46:37.9
18:15:38.00 +37:10:50.0
18:16:57.91 +36:56:40.3
18:26:25.54 +37:25:40.5
18:18:43.97 +36:27:44.8
18:23:08.03 +35:49:54.8
18:20:24.01 +36:09:20.1
18:20:19.59 +35:15:32.3
18:15:22.99 +37:18:15.1
18:22:56.36 +35:56:58.7
18:26:55.22 +37:08:05.7
18:21:56.21 +36:31:39.2
18:20:15.59 +35:01:33.2
18:12:31.18 +38:16:08.6
18:27:47.72 +36:09:51.1
18:22:02.51 +35:13:38.4
18:15:56.36 +36:57:03.1
18:20:44.69 +34:59:48.5
18:20:12.76 +35:03:37.0
18:20:55.49 +35:46:50.2
18:20:02.08 +35:34:42.9
18:20:16.40 +35:10:53.1
18:19:58.80 +35:52:40.9
18:19:35.15 +35:11:24.0
18:27:38.95 +36:52:32.1
18:21:18.87 +35:03:38.1
18:20:58.35 +36:10:37.0
18:26:22.68 +37:25:58.6
18:20:35.38 +36:10:32.0
18:19:56.00 +35:03:14.1
18:26:07.17 +37:28:48.5
18:19:37.36 +35:05:18.7
18:19:57.45 +36:14:17.2
18:21:44.02 +35:28:26.2
18:26:50.38 +36:25:27.4
18:20:14.77 +36:17:13.4
18:21:39.39 +35:36:42.5
18:20:58.88 +36:05:50.3
18:19:39.78 +35:55:12.1
18:22:28.47 +35:30:41.5
18:20:05.05 +36:20:11.6
18:16:20.70 +37:03:22.8
18:26:38.99 +36:29:21.1
18:19:07.29 +36:34:37.9
18:19:59.20 +35:12:34.7
18:26:10.02 +37:25:31.9
18:22:11.65 +35:45:27.2
18:19:39.70 +35:05:43.0
18:28:12.22 +36:17:47.5
18:20:28.81 +36:08:37.9
18:21:05.44 +35:34:18.6
18:16:38.63 +37:07:34.1
18:20:08.23 +35:05:07.3
18:20:10.13 +35:36:44.6
18:23:48.96 +35:48:39.9
18:21:20.68 +35:00:44.7
18:20:56.48 +35:10:45.4
18:18:46.29 +36:31:17.3
18:21:05.80 +36:03:22.3
18:20:35.26 +35:55:01.5
18:20:52.29 +35:01:34.3
18:20:09.14 +35:07:53.0
18:20:15.86 +35:43:55.0
18:20:59.23 +36:09:09.9
18:18:16.25 +36:31:49.8
18:26:34.05 +36:52:02.1
18:26:09.35 +36:30:32.5
18:21:24.59 +35:06:19.7
18:26:19.58 +36:40:05.0
18:21:38.96 +35:14:57.1
18:19:35.89 +36:17:49.0
18:19:17.44 +35:16:42.8
18:18:25.71 +36:35:10.4
18:25:55.58 +37:02:24.6
18:21:59.21 +36:04:36.7
18:17:43.21 +36:46:57.2
18:24:51.53 +36:33:42.8
18:25:48.28 +36:48:27.2
18:21:17.23 +35:50:46.1
18:17:55.89 +36:38:09.6
18:16:39.70 +36:56:22.8
18:20:09.53 +35:45:59.8
18:19:33.35 +35:23:16.9
18:21:06.66 +36:16:57.2
18:20:52.60 +35:09:51.5
18:20:42.19 +36:10:54.9
18:27:36.25 +36:59:42.3
18:17:33.87 +36:42:58.2
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18:23:51.35 +35:49:26.9
18:21:53.41 +35:11:15.3
18:20:25.31 +35:10:55.1
18:19:46.79 +35:11:40.0
18:20:17.88 +35:17:23.6
18:22:06.95 +35:10:40.0
18:20:11.40 +35:17:12.1
18:20:32.04 +35:15:23.7
18:22:04.90 +34:57:58.9
18:27:15.54 +36:12:12.6
18:20:09.66 +35:02:50.1
18:19:28.59 +35:57:54.6
18:18:00.07 +36:50:12.1
18:19:32.80 +35:06:08.5
18:25:29.17 +36:32:12.6
18:20:33.60 +35:43:43.7
18:20:43.68 +35:44:26.9
18:18:12.38 +36:32:10.8
18:20:32.77 +35:25:08.5
18:21:31.45 +36:04:17.8
18:20:01.26 +35:18:18.1
18:17:11.95 +37:10:04.0
18:20:07.78 +35:03:31.2
18:19:23.12 +35:14:06.5
18:20:55.53 +35:57:41.0
18:19:21.78 +35:46:52.2
18:21:02.95 +35:55:38.0
18:16:29.88 +37:00:31.6
18:22:06.38 +35:07:35.9
18:20:19.67 +35:53:11.7
18:17:51.07 +36:40:45.5
18:20:52.79 +35:56:37.0
18:21:43.51 +34:53:21.6
18:19:54.93 +36:25:00.8
18:20:09.35 +36:20:02.1
18:19:43.46 +36:00:36.9
18:26:58.78 +36:47:15.0
18:18:39.82 +36:28:28.7
18:21:46.48 +35:02:24.0
18:15:40.41 +37:06:14.1
18:17:07.83 +36:51:40.7
18:20:17.13 +35:56:40.0
18:16:28.59 +36:58:45.7
18:21:17.39 +35:03:52.7
18:27:56.66 +36:23:24.0
18:19:36.53 +36:30:54.3
18:21:42.28 +35:45:08.3
18:21:21.19 +35:18:41.3
18:26:13.77 +36:59:13.5
18:20:44.26 +36:10:32.8
18:17:41.34 +36:48:19.6
18:20:51.60 +35:06:31.8
18:18:41.96 +36:39:05.2
18:17:37.36 +36:37:17.3
18:20:27.60 +35:35:25.4
18:21:02.14 +35:11:59.1
18:21:54.62 +34:51:53.7
18:19:55.32 +35:15:00.1
18:20:49.28 +35:55:21.2
18:19:30.30 +35:08:53.2
18:19:58.01 +35:58:15.6
18:18:06.54 +36:35:11.0
18:17:11.10 +36:50:42.1
18:20:07.81 +35:01:52.7
18:21:21.37 +36:11:25.2
18:19:38.31 +35:54:42.7
18:20:17.51 +35:46:15.0
18:19:52.56 +35:57:21.6
18:27:19.20 +37:15:39.5
18:20:19.40 +36:16:23.6
18:19:32.11 +36:12:43.4
18:21:20.47 +35:35:19.5
18:26:49.82 +36:53:36.3
18:18:45.52 +33:47:29.8
18:16:45.28 +36:56:58.9
18:15:59.65 +37:06:40.5
18:17:17.50 +36:55:05.1
18:19:45.92 +35:09:32.1
18:20:45.35 +35:12:54.8
18:20:48.12 +36:06:49.9
18:20:50.39 +35:53:03.5
18:17:22.82 +36:37:13.8
18:21:57.01 +35:59:21.1
18:23:52.95 +37:06:52.9
18:26:33.88 +37:01:21.9
18:20:38.44 +35:53:23.9
18:22:17.46 +36:03:34.7
18:21:38.25 +35:00:00.4
18:21:41.25 +35:02:37.6
18:20:41.77 +35:36:27.3
18:15:48.38 +37:11:13.6
18:20:29.66 +35:41:56.9
18:17:18.34 +36:45:48.0
18:27:59.95 +36:49:13.0
18:16:32.23 +37:01:22.6
18:20:12.10 +36:02:51.4
18:21:05.85 +35:51:42.5
18:20:31.97 +35:43:18.5
18:26:24.92 +37:11:09.6
18:17:23.88 +36:37:51.5
18:26:04.21 +37:03:38.3
18:20:45.14 +35:07:21.2
18:20:02.21 +36:07:33.7
18:28:14.94 +36:18:47.9
18:19:51.15 +35:35:05.2
18:16:55.14 +36:36:41.9
18:21:38.73 +35:06:39.7
18:26:53.88 +36:55:50.0
18:26:35.10 +36:31:43.2
18:21:08.16 +36:00:06.7
18:17:41.10 +36:50:46.7
18:17:10.84 +36:51:27.8
18:18:36.64 +36:34:56.4
18:26:15.52 +36:30:44.3
18:19:46.07 +36:07:22.6
18:17:20.05 +36:46:50.9
18:27:29.01 +36:11:44.6
18:20:17.29 +35:06:44.5
18:19:21.79 +35:31:11.9
18:20:18.12 +36:21:07.3
18:24:33.46 +37:22:21.6
18:22:11.20 +35:39:36.5
18:20:25.92 +36:19:43.6
18:17:01.30 +36:50:58.5
18:22:03.95 +35:47:58.2
18:20:58.03 +35:06:31.0
18:20:26.19 +35:05:09.8
18:20:31.43 +36:08:32.3
18:18:02.06 +36:54:14.0
18:19:16.50 +35:22:55.7
18:22:53.10 +35:46:21.5
18:23:10.68 +35:53:25.6
18:21:32.47 +35:05:01.3
18:26:02.91 +36:30:46.2
18:20:43.45 +35:46:58.4
18:20:09.86 +35:05:25.9
18:16:48.82 +37:09:26.1
18:25:42.68 +39:17:45.6
18:14:43.24 +37:19:17.3
18:21:14.20 +35:06:38.9
18:27:26.25 +36:27:37.9
18:20:51.13 +35:53:57.9
18:27:02.28 +36:32:23.1
18:20:56.60 +35:13:04.7
18:20:11.78 +36:12:01.9
18:21:09.78 +36:08:39.4
###################################################################################
18:26:57.73 +37:09:48.1 -- not an asteroid (will add it to exclusion list)
18:17:16.34 +36:53:47.6 -- not an asteroid (will add it to exclusion list)
18:20:29.47 +35:43:37.3 -- not an asteroid (will add it to exclusion list)
18:26:30.95 +36:58:23.7 -- not an asteroid (will add it to exclusion list)
18:27:47.76 +36:34:36.4 -- not an asteroid (will add it to exclusion list)
18:21:38.39 +35:22:32.0 -- not an asteroid (will add it to exclusion list)
18:19:18.84 +35:15:31.9 -- not an asteroid (will add it to exclusion list)
18:22:54.85 +36:00:21.0 -- not an asteroid (will add it to exclusion list)
18:18:59.79 +36:30:15.6 -- not an asteroid (will add it to exclusion list)
18:17:36.21 +36:45:23.8 -- not an asteroid (will add it to exclusion list)
18:20:36.82 +35:07:35.9 -- not an asteroid (will add it to exclusion list)
18:17:54.65 +36:47:19.7 -- not an asteroid (will add it to exclusion list)
18:13:41.80 +37:57:28.6 -- not an asteroid (will add it to exclusion list)
18:16:47.46 +36:50:30.6 -- not an asteroid (will add it to exclusion list)
18:32:54.76 +39:03:22.7 -- not an asteroid (will add it to exclusion list)
18:26:45.08 +36:52:48.1 -- not an asteroid (will add it to exclusion list)
18:21:06.43 +35:05:07.3 -- not an asteroid (will add it to exclusion list)
18:20:25.35 +34:59:41.3 -- not an asteroid (will add it to exclusion list)
18:20:54.04 +35:55:49.0 -- not an asteroid (will add it to exclusion list)
18:20:47.00 +36:05:52.4 -- not an asteroid (will add it to exclusion list)
18:20:01.37 +36:18:36.7 -- not an asteroid (will add it to exclusion list)
18:26:09.97 +36:58:52.6 -- not an asteroid (will add it to exclusion list)
18:26:03.15 +37:37:41.7 -- not an asteroid (will add it to exclusion list)
18:25:56.89 +37:04:27.0 -- not an asteroid (will add it to exclusion list)
18:20:02.39 +35:15:47.5 -- not an asteroid (will add it to exclusion list)
18:19:59.42 +35:56:26.6 -- not an asteroid (will add it to exclusion list)
18:13:33.91 +37:31:28.1 -- not an asteroid (will add it to exclusion list)
18:26:56.02 +36:37:39.4 -- not an asteroid (will add it to exclusion list)
18:28:25.53 +36:15:34.4 -- not an asteroid (will add it to exclusion list)
18:16:26.75 +36:45:38.6 -- not an asteroid (will add it to exclusion list)
18:14:15.76 +37:22:54.7 -- not an asteroid (will add it to exclusion list)
18:17:24.41 +36:43:56.8 -- not an asteroid (will add it to exclusion list)
18:38:07.84 +37:38:16.8 -- not an asteroid (will add it to exclusion list)
18:20:36.57 +36:17:20.7 -- not an asteroid (will add it to exclusion list)
18:21:40.01 +35:09:46.6 -- not an asteroid (will add it to exclusion list)
18:24:06.76 +37:13:19.9 -- not an asteroid (will add it to exclusion list)
18:19:48.26 +36:08:50.6 -- not an asteroid (will add it to exclusion list)
18:20:48.09 +35:43:33.7 -- not an asteroid (will add it to exclusion list)
18:26:04.39 +37:34:52.4 -- not an asteroid (will add it to exclusion list)
18:26:36.99 +36:57:29.7 -- not an asteroid (will add it to exclusion list)
18:20:23.73 +36:25:30.8 -- not an asteroid (will add it to exclusion list)
18:21:11.00 +35:13:38.5 -- not an asteroid (will add it to exclusion list)
18:17:17.28 +36:50:22.7 -- not an asteroid (will add it to exclusion list)
18:22:17.09 +36:00:29.1 -- not an asteroid (will add it to exclusion list)
18:22:44.76 +35:34:27.0 -- not an asteroid (will add it to exclusion list)
18:28:25.39 +37:15:31.4 -- not an asteroid (will add it to exclusion list)
18:16:34.78 +36:56:15.8 -- not an asteroid (will add it to exclusion list)
18:25:36.73 +37:24:42.1 -- not an asteroid (will add it to exclusion list)
18:19:03.60 +36:33:07.4 -- not an asteroid (will add it to exclusion list)
18:16:33.62 +36:47:32.1 -- not an asteroid (will add it to exclusion list)
18:16:28.94 +36:44:54.8 -- not an asteroid (will add it to exclusion list)
18:16:52.13 +36:49:12.6 -- not an asteroid (will add it to exclusion list)
18:21:58.83 +35:07:13.8 -- not an asteroid (will add it to exclusion list)
18:18:34.80 +36:32:53.2 -- not an asteroid (will add it to exclusion list)
18:18:19.52 +36:42:13.7 -- not an asteroid (will add it to exclusion list)
18:16:35.00 +37:08:31.9 -- not an asteroid (will add it to exclusion list)
18:25:41.48 +37:36:35.3 -- not an asteroid (will add it to exclusion list)
18:21:54.73 +34:56:11.3 -- not an asteroid (will add it to exclusion list)
18:20:33.25 +35:49:00.3 -- not an asteroid (will add it to exclusion list)
18:16:45.02 +36:54:47.1 -- not an asteroid (will add it to exclusion list)
18:20:05.97 +35:20:47.7 -- not an asteroid (will add it to exclusion list)
18:17:57.78 +36:46:05.5 -- not an asteroid (will add it to exclusion list)
18:26:48.51 +37:30:11.4 -- not an asteroid (will add it to exclusion list)
18:19:27.19 +34:05:16.3 -- not an asteroid (will add it to exclusion list)
18:16:54.48 +37:03:34.5 -- not an asteroid (will add it to exclusion list)
18:19:48.94 +35:12:14.2 -- not an asteroid (will add it to exclusion list)
18:26:40.54 +36:34:19.4 -- not an asteroid (will add it to exclusion list)
18:15:07.75 +37:16:07.9 -- not an asteroid (will add it to exclusion list)
18:17:32.96 +36:28:15.7 -- not an asteroid (will add it to exclusion list)
18:26:43.33 +37:15:35.8 -- not an asteroid (will add it to exclusion list)
18:26:06.96 +37:14:57.3 -- not an asteroid (will add it to exclusion list)
18:18:53.44 +36:02:17.5 -- not an asteroid (will add it to exclusion list)
18:25:27.50 +37:16:23.3 -- not an asteroid (will add it to exclusion list)
18:15:48.09 +37:12:21.0 -- not an asteroid (will add it to exclusion list)
18:20:04.91 +35:14:38.9 -- not an asteroid (will add it to exclusion list)
18:17:33.42 +36:47:07.2 -- not an asteroid (will add it to exclusion list)
18:19:11.28 +36:30:14.4 -- not an asteroid (will add it to exclusion list)
18:20:55.56 +35:10:33.8 -- not an asteroid (will add it to exclusion list)
18:18:16.08 +36:37:46.4 -- not an asteroid (will add it to exclusion list)
18:21:34.99 +35:37:40.3 -- not an asteroid (will add it to exclusion list)
18:20:55.76 +35:45:50.3 -- not an asteroid (will add it to exclusion list)
18:18:38.25 +36:37:42.2 -- not an asteroid (will add it to exclusion list)
18:20:05.29 +35:28:00.2 -- not an asteroid (will add it to exclusion list)
18:16:14.04 +36:50:13.6 -- not an asteroid (will add it to exclusion list)
18:22:28.74 +35:48:07.7 -- not an asteroid (will add it to exclusion list)
18:20:22.59 +35:58:12.7 -- not an asteroid (will add it to exclusion list)
18:17:17.24 +36:42:08.8 -- not an asteroid (will add it to exclusion list)
18:22:06.80 +35:57:17.6 -- not an asteroid (will add it to exclusion list)
18:26:43.57 +36:59:14.0 -- not an asteroid (will add it to exclusion list)
18:22:21.77 +34:54:00.4 -- not an asteroid (will add it to exclusion list)
18:19:30.44 +35:01:38.3 -- not an asteroid (will add it to exclusion list)
18:21:07.98 +35:46:37.9 -- not an asteroid (will add it to exclusion list)
18:15:38.00 +37:10:50.0 -- not an asteroid (will add it to exclusion list)
18:16:57.91 +36:56:40.3 -- not an asteroid (will add it to exclusion list)
18:26:25.54 +37:25:40.5 -- not an asteroid (will add it to exclusion list)
18:18:43.97 +36:27:44.8 -- not an asteroid (will add it to exclusion list)
18:23:08.03 +35:49:54.8 -- not an asteroid (will add it to exclusion list)
18:20:24.01 +36:09:20.1 -- not an asteroid (will add it to exclusion list)
18:20:19.59 +35:15:32.3 -- not an asteroid (will add it to exclusion list)
18:15:22.99 +37:18:15.1 -- not an asteroid (will add it to exclusion list)
18:22:56.36 +35:56:58.7 -- not an asteroid (will add it to exclusion list)
18:26:55.22 +37:08:05.7 -- not an asteroid (will add it to exclusion list)
18:21:56.21 +36:31:39.2 -- not an asteroid (will add it to exclusion list)
18:20:15.59 +35:01:33.2 -- not an asteroid (will add it to exclusion list)
18:12:31.18 +38:16:08.6 -- not an asteroid (will add it to exclusion list)
18:27:47.72 +36:09:51.1 -- not an asteroid (will add it to exclusion list)
18:22:02.51 +35:13:38.4 -- not an asteroid (will add it to exclusion list)
18:15:56.36 +36:57:03.1 -- not an asteroid (will add it to exclusion list)
18:20:44.69 +34:59:48.5 -- not an asteroid (will add it to exclusion list)
18:20:12.76 +35:03:37.0 -- not an asteroid (will add it to exclusion list)
18:20:55.49 +35:46:50.2 -- not an asteroid (will add it to exclusion list)
18:20:02.08 +35:34:42.9 -- not an asteroid (will add it to exclusion list)
18:20:16.40 +35:10:53.1 -- not an asteroid (will add it to exclusion list)
18:19:58.80 +35:52:40.9 -- not an asteroid (will add it to exclusion list)
18:19:35.15 +35:11:24.0 -- not an asteroid (will add it to exclusion list)
18:27:38.95 +36:52:32.1 -- not an asteroid (will add it to exclusion list)
18:21:18.87 +35:03:38.1 -- not an asteroid (will add it to exclusion list)
18:20:58.35 +36:10:37.0 -- not an asteroid (will add it to exclusion list)
18:26:22.68 +37:25:58.6 -- not an asteroid (will add it to exclusion list)
18:20:35.38 +36:10:32.0 -- not an asteroid (will add it to exclusion list)
18:19:56.00 +35:03:14.1 -- not an asteroid (will add it to exclusion list)
18:26:07.17 +37:28:48.5 -- not an asteroid (will add it to exclusion list)
18:19:37.36 +35:05:18.7 -- not an asteroid (will add it to exclusion list)
18:19:57.45 +36:14:17.2 -- not an asteroid (will add it to exclusion list)
18:21:44.02 +35:28:26.2 -- not an asteroid (will add it to exclusion list)
18:26:50.38 +36:25:27.4 -- not an asteroid (will add it to exclusion list)
18:20:14.77 +36:17:13.4 -- not an asteroid (will add it to exclusion list)
18:21:39.39 +35:36:42.5 -- not an asteroid (will add it to exclusion list)
18:20:58.88 +36:05:50.3 -- not an asteroid (will add it to exclusion list)
18:19:39.78 +35:55:12.1 -- not an asteroid (will add it to exclusion list)
18:22:28.47 +35:30:41.5 -- not an asteroid (will add it to exclusion list)
18:20:05.05 +36:20:11.6 -- not an asteroid (will add it to exclusion list)
18:16:20.70 +37:03:22.8 -- not an asteroid (will add it to exclusion list)
18:26:38.99 +36:29:21.1 -- not an asteroid (will add it to exclusion list)
18:19:07.29 +36:34:37.9 -- not an asteroid (will add it to exclusion list)
18:19:59.20 +35:12:34.7 -- not an asteroid (will add it to exclusion list)
18:26:10.02 +37:25:31.9 -- not an asteroid (will add it to exclusion list)
18:22:11.65 +35:45:27.2 -- not an asteroid (will add it to exclusion list)
18:19:39.70 +35:05:43.0 -- not an asteroid (will add it to exclusion list)
18:28:12.22 +36:17:47.5 -- not an asteroid (will add it to exclusion list)
18:20:28.81 +36:08:37.9 -- not an asteroid (will add it to exclusion list)
18:21:05.44 +35:34:18.6 -- not an asteroid (will add it to exclusion list)
18:16:38.63 +37:07:34.1 -- not an asteroid (will add it to exclusion list)
18:20:08.23 +35:05:07.3 -- not an asteroid (will add it to exclusion list)
18:20:10.13 +35:36:44.6 -- not an asteroid (will add it to exclusion list)
18:23:48.96 +35:48:39.9 -- not an asteroid (will add it to exclusion list)
18:21:20.68 +35:00:44.7 -- not an asteroid (will add it to exclusion list)
18:20:56.48 +35:10:45.4 -- not an asteroid (will add it to exclusion list)
18:18:46.29 +36:31:17.3 -- not an asteroid (will add it to exclusion list)
18:21:05.80 +36:03:22.3 -- not an asteroid (will add it to exclusion list)
18:20:35.26 +35:55:01.5 -- not an asteroid (will add it to exclusion list)
18:20:52.29 +35:01:34.3 -- not an asteroid (will add it to exclusion list)
18:20:09.14 +35:07:53.0 -- not an asteroid (will add it to exclusion list)
18:20:15.86 +35:43:55.0 -- not an asteroid (will add it to exclusion list)
18:20:59.23 +36:09:09.9 -- not an asteroid (will add it to exclusion list)
18:18:16.25 +36:31:49.8 -- not an asteroid (will add it to exclusion list)
18:26:34.05 +36:52:02.1 -- not an asteroid (will add it to exclusion list)
18:26:09.35 +36:30:32.5 -- not an asteroid (will add it to exclusion list)
18:21:24.59 +35:06:19.7 -- not an asteroid (will add it to exclusion list)
18:26:19.58 +36:40:05.0 -- not an asteroid (will add it to exclusion list)
18:21:38.96 +35:14:57.1 -- not an asteroid (will add it to exclusion list)
18:19:35.89 +36:17:49.0 -- not an asteroid (will add it to exclusion list)
18:19:17.44 +35:16:42.8 -- not an asteroid (will add it to exclusion list)
18:18:25.71 +36:35:10.4 -- not an asteroid (will add it to exclusion list)
18:25:55.58 +37:02:24.6 -- not an asteroid (will add it to exclusion list)
18:21:59.21 +36:04:36.7 -- not an asteroid (will add it to exclusion list)
18:17:43.21 +36:46:57.2 -- not an asteroid (will add it to exclusion list)
18:24:51.53 +36:33:42.8 -- not an asteroid (will add it to exclusion list)
18:25:48.28 +36:48:27.2 -- not an asteroid (will add it to exclusion list)
18:21:17.23 +35:50:46.1 -- not an asteroid (will add it to exclusion list)
18:17:55.89 +36:38:09.6 -- not an asteroid (will add it to exclusion list)
18:16:39.70 +36:56:22.8 -- not an asteroid (will add it to exclusion list)
18:20:09.53 +35:45:59.8 -- not an asteroid (will add it to exclusion list)
18:19:33.35 +35:23:16.9 -- not an asteroid (will add it to exclusion list)
18:21:06.66 +36:16:57.2 -- not an asteroid (will add it to exclusion list)
18:20:52.60 +35:09:51.5 -- not an asteroid (will add it to exclusion list)
18:20:42.19 +36:10:54.9 -- not an asteroid (will add it to exclusion list)
18:27:36.25 +36:59:42.3 -- not an asteroid (will add it to exclusion list)
18:17:33.87 +36:42:58.2 -- not an asteroid (will add it to exclusion list)
18:20:16.18 +34:59:55.1 -- not an asteroid (will add it to exclusion list)
18:23:51.35 +35:49:26.9 -- not an asteroid (will add it to exclusion list)
18:21:53.41 +35:11:15.3 -- not an asteroid (will add it to exclusion list)
18:20:25.31 +35:10:55.1 -- not an asteroid (will add it to exclusion list)
18:19:46.79 +35:11:40.0 -- not an asteroid (will add it to exclusion list)
18:20:17.88 +35:17:23.6 -- not an asteroid (will add it to exclusion list)
18:22:06.95 +35:10:40.0 -- not an asteroid (will add it to exclusion list)
18:20:11.40 +35:17:12.1 -- not an asteroid (will add it to exclusion list)
18:20:32.04 +35:15:23.7 -- not an asteroid (will add it to exclusion list)
18:22:04.90 +34:57:58.9 -- not an asteroid (will add it to exclusion list)
18:27:15.54 +36:12:12.6 -- not an asteroid (will add it to exclusion list)
18:20:09.66 +35:02:50.1 -- not an asteroid (will add it to exclusion list)
18:19:28.59 +35:57:54.6 -- not an asteroid (will add it to exclusion list)
18:18:00.07 +36:50:12.1 -- not an asteroid (will add it to exclusion list)
18:19:32.80 +35:06:08.5 -- not an asteroid (will add it to exclusion list)
18:25:29.17 +36:32:12.6 -- not an asteroid (will add it to exclusion list)
18:20:33.60 +35:43:43.7 -- not an asteroid (will add it to exclusion list)
18:20:43.68 +35:44:26.9 -- not an asteroid (will add it to exclusion list)
18:18:12.38 +36:32:10.8 -- not an asteroid (will add it to exclusion list)
18:20:32.77 +35:25:08.5 -- not an asteroid (will add it to exclusion list)
18:21:31.45 +36:04:17.8 -- not an asteroid (will add it to exclusion list)
18:20:01.26 +35:18:18.1 -- not an asteroid (will add it to exclusion list)
18:17:11.95 +37:10:04.0 -- not an asteroid (will add it to exclusion list)
18:20:07.78 +35:03:31.2 -- not an asteroid (will add it to exclusion list)
18:19:23.12 +35:14:06.5 -- not an asteroid (will add it to exclusion list)
18:20:55.53 +35:57:41.0 -- not an asteroid (will add it to exclusion list)
18:19:21.78 +35:46:52.2 -- not an asteroid (will add it to exclusion list)
18:21:02.95 +35:55:38.0 -- not an asteroid (will add it to exclusion list)
18:16:29.88 +37:00:31.6 -- not an asteroid (will add it to exclusion list)
18:22:06.38 +35:07:35.9 -- not an asteroid (will add it to exclusion list)
18:20:19.67 +35:53:11.7 -- not an asteroid (will add it to exclusion list)
18:17:51.07 +36:40:45.5 -- not an asteroid (will add it to exclusion list)
18:20:52.79 +35:56:37.0 -- not an asteroid (will add it to exclusion list)
18:21:43.51 +34:53:21.6 -- not an asteroid (will add it to exclusion list)
18:19:54.93 +36:25:00.8 -- not an asteroid (will add it to exclusion list)
18:20:09.35 +36:20:02.1 -- not an asteroid (will add it to exclusion list)
18:19:43.46 +36:00:36.9 -- not an asteroid (will add it to exclusion list)
18:26:58.78 +36:47:15.0 -- not an asteroid (will add it to exclusion list)
18:18:39.82 +36:28:28.7 -- not an asteroid (will add it to exclusion list)
18:21:46.48 +35:02:24.0 -- not an asteroid (will add it to exclusion list)
18:15:40.41 +37:06:14.1 -- not an asteroid (will add it to exclusion list)
18:17:07.83 +36:51:40.7 -- not an asteroid (will add it to exclusion list)
18:20:17.13 +35:56:40.0 -- not an asteroid (will add it to exclusion list)
18:16:28.59 +36:58:45.7 -- not an asteroid (will add it to exclusion list)
18:21:17.39 +35:03:52.7 -- not an asteroid (will add it to exclusion list)
18:27:56.66 +36:23:24.0 -- not an asteroid (will add it to exclusion list)
18:19:36.53 +36:30:54.3 -- not an asteroid (will add it to exclusion list)
18:21:42.28 +35:45:08.3 -- not an asteroid (will add it to exclusion list)
18:21:21.19 +35:18:41.3 -- not an asteroid (will add it to exclusion list)
18:26:13.77 +36:59:13.5 -- not an asteroid (will add it to exclusion list)
18:20:44.26 +36:10:32.8 -- not an asteroid (will add it to exclusion list)
18:17:41.34 +36:48:19.6 -- not an asteroid (will add it to exclusion list)
18:20:51.60 +35:06:31.8 -- not an asteroid (will add it to exclusion list)
18:18:41.96 +36:39:05.2 -- not an asteroid (will add it to exclusion list)
18:17:37.36 +36:37:17.3 -- not an asteroid (will add it to exclusion list)
18:20:27.60 +35:35:25.4 -- not an asteroid (will add it to exclusion list)
18:21:02.14 +35:11:59.1 -- not an asteroid (will add it to exclusion list)
18:21:54.62 +34:51:53.7 -- not an asteroid (will add it to exclusion list)
18:19:55.32 +35:15:00.1 -- not an asteroid (will add it to exclusion list)
18:20:49.28 +35:55:21.2 -- not an asteroid (will add it to exclusion list)
18:19:30.30 +35:08:53.2 -- not an asteroid (will add it to exclusion list)
18:19:58.01 +35:58:15.6 -- not an asteroid (will add it to exclusion list)
18:18:06.54 +36:35:11.0 -- not an asteroid (will add it to exclusion list)
18:17:11.10 +36:50:42.1 -- not an asteroid (will add it to exclusion list)
18:20:07.81 +35:01:52.7 -- not an asteroid (will add it to exclusion list)
18:21:21.37 +36:11:25.2 -- not an asteroid (will add it to exclusion list)
18:19:38.31 +35:54:42.7 -- not an asteroid (will add it to exclusion list)
18:20:17.51 +35:46:15.0 -- not an asteroid (will add it to exclusion list)
18:19:52.56 +35:57:21.6 -- not an asteroid (will add it to exclusion list)
18:27:19.20 +37:15:39.5 -- not an asteroid (will add it to exclusion list)
18:20:19.40 +36:16:23.6 -- not an asteroid (will add it to exclusion list)
18:19:32.11 +36:12:43.4 -- not an asteroid (will add it to exclusion list)
18:21:20.47 +35:35:19.5 -- not an asteroid (will add it to exclusion list)
18:26:49.82 +36:53:36.3 -- not an asteroid (will add it to exclusion list)
18:18:45.52 +33:47:29.8 -- not an asteroid (will add it to exclusion list)
18:16:45.28 +36:56:58.9 -- not an asteroid (will add it to exclusion list)
18:15:59.65 +37:06:40.5 -- not an asteroid (will add it to exclusion list)
18:17:17.50 +36:55:05.1 -- not an asteroid (will add it to exclusion list)
18:19:45.92 +35:09:32.1 -- not an asteroid (will add it to exclusion list)
18:20:45.35 +35:12:54.8 -- not an asteroid (will add it to exclusion list)
18:20:48.12 +36:06:49.9 -- not an asteroid (will add it to exclusion list)
18:20:50.39 +35:53:03.5 -- not an asteroid (will add it to exclusion list)
18:17:22.82 +36:37:13.8 -- not an asteroid (will add it to exclusion list)
18:21:57.01 +35:59:21.1 -- not an asteroid (will add it to exclusion list)
18:23:52.95 +37:06:52.9 -- not an asteroid (will add it to exclusion list)
18:26:33.88 +37:01:21.9 -- not an asteroid (will add it to exclusion list)
18:20:38.44 +35:53:23.9 -- not an asteroid (will add it to exclusion list)
18:22:17.46 +36:03:34.7 -- not an asteroid (will add it to exclusion list)
18:21:38.25 +35:00:00.4 -- not an asteroid (will add it to exclusion list)
18:21:41.25 +35:02:37.6 -- not an asteroid (will add it to exclusion list)
18:20:41.77 +35:36:27.3 -- not an asteroid (will add it to exclusion list)
18:15:48.38 +37:11:13.6 -- not an asteroid (will add it to exclusion list)
18:20:29.66 +35:41:56.9 -- not an asteroid (will add it to exclusion list)
18:17:18.34 +36:45:48.0 -- not an asteroid (will add it to exclusion list)
18:27:59.95 +36:49:13.0 -- not an asteroid (will add it to exclusion list)
18:16:32.23 +37:01:22.6 -- not an asteroid (will add it to exclusion list)
18:20:12.10 +36:02:51.4 -- not an asteroid (will add it to exclusion list)
18:21:05.85 +35:51:42.5 -- not an asteroid (will add it to exclusion list)
18:20:31.97 +35:43:18.5 -- not an asteroid (will add it to exclusion list)
18:26:24.92 +37:11:09.6 -- not an asteroid (will add it to exclusion list)
18:17:23.88 +36:37:51.5 -- not an asteroid (will add it to exclusion list)
18:26:04.21 +37:03:38.3 -- not an asteroid (will add it to exclusion list)
18:20:45.14 +35:07:21.2 -- not an asteroid (will add it to exclusion list)
18:20:02.21 +36:07:33.7 -- not an asteroid (will add it to exclusion list)
18:28:14.94 +36:18:47.9 -- not an asteroid (will add it to exclusion list)
18:19:51.15 +35:35:05.2 -- not an asteroid (will add it to exclusion list)
18:16:55.14 +36:36:41.9 -- not an asteroid (will add it to exclusion list)
18:21:38.73 +35:06:39.7 -- not an asteroid (will add it to exclusion list)
18:26:53.88 +36:55:50.0 -- not an asteroid (will add it to exclusion list)
18:26:35.10 +36:31:43.2 -- not an asteroid (will add it to exclusion list)
18:21:08.16 +36:00:06.7 -- not an asteroid (will add it to exclusion list)
18:17:41.10 +36:50:46.7 -- not an asteroid (will add it to exclusion list)
18:17:10.84 +36:51:27.8 -- not an asteroid (will add it to exclusion list)
18:18:36.64 +36:34:56.4 -- not an asteroid (will add it to exclusion list)
18:26:15.52 +36:30:44.3 -- not an asteroid (will add it to exclusion list)
18:19:46.07 +36:07:22.6 -- not an asteroid (will add it to exclusion list)
18:17:20.05 +36:46:50.9 -- not an asteroid (will add it to exclusion list)
18:27:29.01 +36:11:44.6 -- not an asteroid (will add it to exclusion list)
18:20:17.29 +35:06:44.5 -- not an asteroid (will add it to exclusion list)
18:19:21.79 +35:31:11.9 -- not an asteroid (will add it to exclusion list)
18:20:18.12 +36:21:07.3 -- not an asteroid (will add it to exclusion list)
18:24:33.46 +37:22:21.6 -- not an asteroid (will add it to exclusion list)
18:22:11.20 +35:39:36.5 -- not an asteroid (will add it to exclusion list)
18:20:25.92 +36:19:43.6 -- not an asteroid (will add it to exclusion list)
18:17:01.30 +36:50:58.5 -- not an asteroid (will add it to exclusion list)
18:22:03.95 +35:47:58.2 -- not an asteroid (will add it to exclusion list)
18:20:58.03 +35:06:31.0 -- not an asteroid (will add it to exclusion list)
18:20:26.19 +35:05:09.8 -- not an asteroid (will add it to exclusion list)
18:20:31.43 +36:08:32.3 -- not an asteroid (will add it to exclusion list)
18:18:02.06 +36:54:14.0 -- not an asteroid (will add it to exclusion list)
18:19:16.50 +35:22:55.7 -- not an asteroid (will add it to exclusion list)
18:22:53.10 +35:46:21.5 -- not an asteroid (will add it to exclusion list)
18:23:10.68 +35:53:25.6 -- not an asteroid (will add it to exclusion list)
18:21:32.47 +35:05:01.3 -- not an asteroid (will add it to exclusion list)
18:26:02.91 +36:30:46.2 -- not an asteroid (will add it to exclusion list)
18:20:43.45 +35:46:58.4 -- not an asteroid (will add it to exclusion list)
18:20:09.86 +35:05:25.9 -- not an asteroid (will add it to exclusion list)
18:16:48.82 +37:09:26.1 -- not an asteroid (will add it to exclusion list)
18:25:42.68 +39:17:45.6 -- not an asteroid (will add it to exclusion list)
18:14:43.24 +37:19:17.3 -- not an asteroid (will add it to exclusion list)
18:21:14.20 +35:06:38.9 -- not an asteroid (will add it to exclusion list)
18:27:26.25 +36:27:37.9 -- not an asteroid (will add it to exclusion list)
18:20:51.13 +35:53:57.9 -- not an asteroid (will add it to exclusion list)
18:27:02.28 +36:32:23.1 -- not an asteroid (will add it to exclusion list)
18:20:56.60 +35:13:04.7 -- not an asteroid (will add it to exclusion list)
18:20:11.78 +36:12:01.9 -- not an asteroid (will add it to exclusion list)
18:21:09.78 +36:08:39.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:12:31.18 +38:16:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:33.91 +37:31:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:41.80 +37:57:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:14:15.76 +37:22:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:14:43.24 +37:19:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:07.75 +37:16:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:22.99 +37:18:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:38.00 +37:10:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:40.41 +37:06:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:48.09 +37:12:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:48.38 +37:11:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:56.36 +36:57:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:59.65 +37:06:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:14.04 +36:50:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:20.70 +37:03:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:26.75 +36:45:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:28.59 +36:58:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:28.94 +36:44:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:29.88 +37:00:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:32.23 +37:01:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:33.62 +36:47:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:34.78 +36:56:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:35.00 +37:08:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:38.63 +37:07:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:39.70 +36:56:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:45.02 +36:54:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:45.28 +36:56:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:47.46 +36:50:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:48.82 +37:09:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:52.13 +36:49:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:54.48 +37:03:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:55.14 +36:36:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:57.91 +36:56:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:01.30 +36:50:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:07.83 +36:51:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:10.84 +36:51:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:11.10 +36:50:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:11.95 +37:10:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:16.34 +36:53:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:17.24 +36:42:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:17.28 +36:50:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:17.50 +36:55:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:18.34 +36:45:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:20.05 +36:46:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:22.82 +36:37:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:23.88 +36:37:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:24.41 +36:43:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:32.96 +36:28:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:33.42 +36:47:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:33.87 +36:42:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:36.21 +36:45:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:37.36 +36:37:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:41.10 +36:50:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:41.34 +36:48:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:43.21 +36:46:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:51.07 +36:40:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:54.65 +36:47:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:55.89 +36:38:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:57.78 +36:46:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:00.07 +36:50:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:02.06 +36:54:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:06.54 +36:35:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:12.38 +36:32:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:16.08 +36:37:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:16.25 +36:31:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:19.52 +36:42:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:25.71 +36:35:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:34.80 +36:32:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:36.64 +36:34:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:38.25 +36:37:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:39.82 +36:28:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:41.96 +36:39:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:43.97 +36:27:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:45.52 +33:47:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:46.29 +36:31:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:53.44 +36:02:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:59.79 +36:30:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:03.60 +36:33:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:07.29 +36:34:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:11.28 +36:30:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:16.50 +35:22:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:17.44 +35:16:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:18.84 +35:15:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:21.78 +35:46:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:21.79 +35:31:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:23.12 +35:14:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:27.19 +34:05:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:28.59 +35:57:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:30.30 +35:08:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:30.44 +35:01:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:32.11 +36:12:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:32.80 +35:06:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:33.35 +35:23:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:35.15 +35:11:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:35.89 +36:17:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:36.53 +36:30:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:37.36 +35:05:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:38.31 +35:54:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:39.70 +35:05:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:39.78 +35:55:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:43.46 +36:00:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:45.92 +35:09:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:46.07 +36:07:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:46.79 +35:11:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:48.26 +36:08:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:48.94 +35:12:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:51.15 +35:35:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:52.56 +35:57:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:54.93 +36:25:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:55.32 +35:15:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:56.00 +35:03:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:57.45 +36:14:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:58.01 +35:58:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:58.80 +35:52:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:59.20 +35:12:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:59.42 +35:56:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:01.26 +35:18:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:01.37 +36:18:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:02.08 +35:34:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:02.21 +36:07:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:02.39 +35:15:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:04.91 +35:14:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:05.05 +36:20:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:05.29 +35:28:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:05.97 +35:20:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:07.78 +35:03:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:07.81 +35:01:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:08.23 +35:05:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:09.14 +35:07:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:09.35 +36:20:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:09.53 +35:45:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:09.66 +35:02:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:09.86 +35:05:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:10.13 +35:36:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:11.40 +35:17:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:11.78 +36:12:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:12.10 +36:02:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:12.76 +35:03:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:14.77 +36:17:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:15.59 +35:01:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:15.86 +35:43:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:16.18 +34:59:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:16.40 +35:10:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:17.13 +35:56:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:17.29 +35:06:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:17.51 +35:46:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:17.88 +35:17:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:18.12 +36:21:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:19.40 +36:16:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:19.59 +35:15:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:19.67 +35:53:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:22.59 +35:58:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:23.73 +36:25:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:24.01 +36:09:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:25.31 +35:10:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:25.35 +34:59:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:25.92 +36:19:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:26.19 +35:05:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:27.60 +35:35:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:28.81 +36:08:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:29.47 +35:43:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:29.66 +35:41:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:31.43 +36:08:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:31.97 +35:43:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:32.04 +35:15:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:32.77 +35:25:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:33.25 +35:49:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:33.60 +35:43:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:35.26 +35:55:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:35.38 +36:10:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:36.57 +36:17:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:36.82 +35:07:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:38.44 +35:53:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:41.77 +35:36:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:42.19 +36:10:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:43.45 +35:46:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:43.68 +35:44:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:44.26 +36:10:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:44.69 +34:59:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:45.14 +35:07:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:45.35 +35:12:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:47.00 +36:05:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:48.09 +35:43:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:48.12 +36:06:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:49.28 +35:55:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:50.39 +35:53:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:51.13 +35:53:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:51.60 +35:06:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:52.29 +35:01:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:52.60 +35:09:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:52.79 +35:56:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:54.04 +35:55:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:55.49 +35:46:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:55.53 +35:57:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:55.56 +35:10:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:55.76 +35:45:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:56.48 +35:10:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:56.60 +35:13:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:58.03 +35:06:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:58.35 +36:10:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:58.88 +36:05:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:59.23 +36:09:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:02.14 +35:11:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:02.95 +35:55:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:05.44 +35:34:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:05.80 +36:03:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:05.85 +35:51:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:06.43 +35:05:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:06.66 +36:16:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:07.98 +35:46:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:08.16 +36:00:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:09.78 +36:08:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:11.00 +35:13:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:14.20 +35:06:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:17.23 +35:50:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:17.39 +35:03:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:18.87 +35:03:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:20.47 +35:35:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:20.68 +35:00:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:21.19 +35:18:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:21.37 +36:11:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:24.59 +35:06:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:31.45 +36:04:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:32.47 +35:05:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:34.99 +35:37:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:38.25 +35:00:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:38.39 +35:22:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:38.73 +35:06:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:38.96 +35:14:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:39.39 +35:36:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:40.01 +35:09:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:41.25 +35:02:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:42.28 +35:45:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:43.51 +34:53:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:44.02 +35:28:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:46.48 +35:02:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:53.41 +35:11:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:54.62 +34:51:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:54.73 +34:56:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:56.21 +36:31:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:57.01 +35:59:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:58.83 +35:07:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:59.21 +36:04:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:02.51 +35:13:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:03.95 +35:47:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:04.90 +34:57:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:06.38 +35:07:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:06.80 +35:57:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:06.95 +35:10:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:11.20 +35:39:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:11.65 +35:45:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:17.09 +36:00:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:17.46 +36:03:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:21.77 +34:54:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:28.47 +35:30:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:28.74 +35:48:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:44.76 +35:34:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:53.10 +35:46:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:54.85 +36:00:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:22:56.36 +35:56:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:23:08.03 +35:49:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:23:10.68 +35:53:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:23:48.96 +35:48:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:23:51.35 +35:49:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:23:52.95 +37:06:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:06.76 +37:13:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:33.46 +37:22:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:51.53 +36:33:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:27.50 +37:16:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:29.17 +36:32:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:36.73 +37:24:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:41.48 +37:36:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:42.68 +39:17:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:48.28 +36:48:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:55.58 +37:02:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:56.89 +37:04:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:02.91 +36:30:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:03.15 +37:37:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:04.21 +37:03:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:04.39 +37:34:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:06.96 +37:14:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:07.17 +37:28:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:09.35 +36:30:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:09.97 +36:58:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:10.02 +37:25:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:13.77 +36:59:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:15.52 +36:30:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:19.58 +36:40:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:22.68 +37:25:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:24.92 +37:11:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:25.54 +37:25:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:30.95 +36:58:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:33.88 +37:01:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:34.05 +36:52:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:35.10 +36:31:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:36.99 +36:57:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:38.99 +36:29:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:40.54 +36:34:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:43.33 +37:15:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:43.57 +36:59:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:45.08 +36:52:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:48.51 +37:30:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:49.82 +36:53:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:50.38 +36:25:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:53.88 +36:55:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:55.22 +37:08:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:56.02 +36:37:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:57.73 +37:09:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:58.78 +36:47:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:02.28 +36:32:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:15.54 +36:12:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:19.20 +37:15:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:26.25 +36:27:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:29.01 +36:11:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:36.25 +36:59:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:38.95 +36:52:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:47.72 +36:09:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:47.76 +36:34:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:56.66 +36:23:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:59.95 +36:49:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:12.22 +36:17:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:14.94 +36:18:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:25.39 +37:15:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:25.53 +36:15:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:32:54.76 +39:03:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:07.84 +37:38:16.8 -- 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)
18:12:31.18 +38:16:08.6 -- not a known variable star
18:13:33.91 +37:31:28.1 -- a known variable star
18:13:41.80 +37:57:28.6 -- not a known variable star
18:14:15.76 +37:22:54.7 -- not a known variable star
18:14:43.24 +37:19:17.3 -- not a known variable star
18:15:07.75 +37:16:07.9 -- not a known variable star
18:15:22.99 +37:18:15.1 -- not a known variable star
18:15:38.00 +37:10:50.0 -- not a known variable star
18:15:40.41 +37:06:14.1 -- not a known variable star
18:15:48.09 +37:12:21.0 -- not a known variable star
18:15:48.38 +37:11:13.6 -- not a known variable star
18:15:56.36 +36:57:03.1 -- not a known variable star
18:15:59.65 +37:06:40.5 -- not a known variable star
18:16:14.04 +36:50:13.6 -- not a known variable star
18:16:20.70 +37:03:22.8 -- not a known variable star
18:16:26.75 +36:45:38.6 -- not a known variable star
18:16:28.59 +36:58:45.7 -- not a known variable star
18:16:28.94 +36:44:54.8 -- a known variable star
18:16:29.88 +37:00:31.6 -- not a known variable star
18:16:32.23 +37:01:22.6 -- not a known variable star
18:16:33.62 +36:47:32.1 -- not a known variable star
18:16:34.78 +36:56:15.8 -- not a known variable star
18:16:35.00 +37:08:31.9 -- not a known variable star
18:16:38.63 +37:07:34.1 -- not a known variable star
18:16:39.70 +36:56:22.8 -- not a known variable star
18:16:45.02 +36:54:47.1 -- not a known variable star
18:16:45.28 +36:56:58.9 -- not a known variable star
18:16:47.46 +36:50:30.6 -- not a known variable star
18:16:48.82 +37:09:26.1 -- not a known variable star
18:16:52.13 +36:49:12.6 -- not a known variable star
18:16:54.48 +37:03:34.5 -- a known variable star
18:16:55.14 +36:36:41.9 -- not a known variable star
18:16:57.91 +36:56:40.3 -- not a known variable star
18:17:01.30 +36:50:58.5 -- not a known variable star
18:17:07.83 +36:51:40.7 -- not a known variable star
18:17:10.84 +36:51:27.8 -- a known variable star
18:17:11.10 +36:50:42.1 -- not a known variable star
18:17:11.95 +37:10:04.0 -- a known variable star
18:17:16.34 +36:53:47.6 -- not a known variable star
18:17:17.24 +36:42:08.8 -- not a known variable star
18:17:17.28 +36:50:22.7 -- a known variable star
18:17:17.50 +36:55:05.1 -- not a known variable star
18:17:18.34 +36:45:48.0 -- a known variable star
18:17:20.05 +36:46:50.9 -- not a known variable star
18:17:22.82 +36:37:13.8 -- not a known variable star
18:17:23.88 +36:37:51.5 -- not a known variable star
18:17:24.41 +36:43:56.8 -- a known variable star
18:17:32.96 +36:28:15.7 -- not a known variable star
18:17:33.42 +36:47:07.2 -- not a known variable star
18:17:33.87 +36:42:58.2 -- not a known variable star
18:17:36.21 +36:45:23.8 -- not a known variable star
18:17:37.36 +36:37:17.3 -- a known variable star
18:17:41.10 +36:50:46.7 -- not a known variable star
18:17:41.34 +36:48:19.6 -- not a known variable star
18:17:43.21 +36:46:57.2 -- not a known variable star
18:17:51.07 +36:40:45.5 -- not a known variable star
18:17:54.65 +36:47:19.7 -- a known variable star
18:17:55.89 +36:38:09.6 -- not a known variable star
18:17:57.78 +36:46:05.5 -- not a known variable star
18:18:00.07 +36:50:12.1 -- not a known variable star
18:18:02.06 +36:54:14.0 -- not a known variable star
18:18:06.54 +36:35:11.0 -- not a known variable star
18:18:12.38 +36:32:10.8 -- not a known variable star
18:18:16.08 +36:37:46.4 -- not a known variable star
18:18:16.25 +36:31:49.8 -- not a known variable star
18:18:19.52 +36:42:13.7 -- not a known variable star
18:18:25.71 +36:35:10.4 -- not a known variable star
18:18:34.80 +36:32:53.2 -- not a known variable star
18:18:36.64 +36:34:56.4 -- not a known variable star
18:18:38.25 +36:37:42.2 -- not a known variable star
18:18:39.82 +36:28:28.7 -- not a known variable star
18:18:41.96 +36:39:05.2 -- not a known variable star
18:18:43.97 +36:27:44.8 -- not a known variable star
18:18:45.52 +33:47:29.8 -- not a known variable star
18:18:46.29 +36:31:17.3 -- a known variable star
18:18:53.44 +36:02:17.5 -- not a known variable star
18:18:59.79 +36:30:15.6 -- not a known variable star
18:19:03.60 +36:33:07.4 -- not a known variable star
18:19:07.29 +36:34:37.9 -- not a known variable star
18:19:11.28 +36:30:14.4 -- not a known variable star
18:19:16.50 +35:22:55.7 -- not a known variable star
18:19:17.44 +35:16:42.8 -- not a known variable star
18:19:18.84 +35:15:31.9 -- not a known variable star
18:19:21.78 +35:46:52.2 -- a known variable star
18:19:21.79 +35:31:11.9 -- not a known variable star
18:19:23.12 +35:14:06.5 -- not a known variable star
18:19:27.19 +34:05:16.3 -- not a known variable star
18:19:28.59 +35:57:54.6 -- not a known variable star
18:19:30.30 +35:08:53.2 -- not a known variable star
18:19:30.44 +35:01:38.3 -- not a known variable star
18:19:32.11 +36:12:43.4 -- not a known variable star
18:19:32.80 +35:06:08.5 -- not a known variable star
18:19:33.35 +35:23:16.9 -- not a known variable star
18:19:35.15 +35:11:24.0 -- not a known variable star
18:19:35.89 +36:17:49.0 -- not a known variable star
18:19:36.53 +36:30:54.3 -- not a known variable star
18:19:37.36 +35:05:18.7 -- not a known variable star
18:19:38.31 +35:54:42.7 -- not a known variable star
18:19:39.70 +35:05:43.0 -- not a known variable star
18:19:39.78 +35:55:12.1 -- not a known variable star
18:19:43.46 +36:00:36.9 -- not a known variable star
18:19:45.92 +35:09:32.1 -- not a known variable star
18:19:46.07 +36:07:22.6 -- not a known variable star
18:19:46.79 +35:11:40.0 -- not a known variable star
18:19:48.26 +36:08:50.6 -- not a known variable star
18:19:48.94 +35:12:14.2 -- not a known variable star
18:19:51.15 +35:35:05.2 -- not a known variable star
18:19:52.56 +35:57:21.6 -- not a known variable star
18:19:54.93 +36:25:00.8 -- not a known variable star
18:19:55.32 +35:15:00.1 -- a known variable star
18:19:56.00 +35:03:14.1 -- not a known variable star
18:19:57.45 +36:14:17.2 -- not a known variable star
18:19:58.01 +35:58:15.6 -- not a known variable star
18:19:58.80 +35:52:40.9 -- a known variable star
18:19:59.20 +35:12:34.7 -- not a known variable star
18:19:59.42 +35:56:26.6 -- not a known variable star
18:20:01.26 +35:18:18.1 -- not a known variable star
18:20:01.37 +36:18:36.7 -- not a known variable star
18:20:02.08 +35:34:42.9 -- not a known variable star
18:20:02.21 +36:07:33.7 -- not a known variable star
18:20:02.39 +35:15:47.5 -- not a known variable star
18:20:04.91 +35:14:38.9 -- a known variable star
18:20:05.05 +36:20:11.6 -- not a known variable star
18:20:05.29 +35:28:00.2 -- not a known variable star
18:20:05.97 +35:20:47.7 -- not a known variable star
18:20:07.78 +35:03:31.2 -- not a known variable star
18:20:07.81 +35:01:52.7 -- not a known variable star
18:20:08.23 +35:05:07.3 -- not a known variable star
18:20:09.14 +35:07:53.0 -- not a known variable star
18:20:09.35 +36:20:02.1 -- not a known variable star
18:20:09.53 +35:45:59.8 -- not a known variable star
18:20:09.66 +35:02:50.1 -- not a known variable star
18:20:09.86 +35:05:25.9 -- not a known variable star
18:20:10.13 +35:36:44.6 -- not a known variable star
18:20:11.40 +35:17:12.1 -- not a known variable star
18:20:11.78 +36:12:01.9 -- not a known variable star
18:20:12.10 +36:02:51.4 -- not a known variable star
18:20:12.76 +35:03:37.0 -- not a known variable star
18:20:14.77 +36:17:13.4 -- not a known variable star
18:20:15.59 +35:01:33.2 -- not a known variable star
18:20:15.86 +35:43:55.0 -- not a known variable star
18:20:16.18 +34:59:55.1 -- not a known variable star
18:20:16.40 +35:10:53.1 -- not a known variable star
18:20:17.13 +35:56:40.0 -- not a known variable star
18:20:17.29 +35:06:44.5 -- not a known variable star
18:20:17.51 +35:46:15.0 -- a known variable star
18:20:17.88 +35:17:23.6 -- not a known variable star
18:20:18.12 +36:21:07.3 -- not a known variable star
18:20:19.40 +36:16:23.6 -- not a known variable star
18:20:19.59 +35:15:32.3 -- not a known variable star
18:20:19.67 +35:53:11.7 -- a known variable star
18:20:22.59 +35:58:12.7 -- not a known variable star
18:20:23.73 +36:25:30.8 -- not a known variable star
18:20:24.01 +36:09:20.1 -- not a known variable star
18:20:25.31 +35:10:55.1 -- not a known variable star
18:20:25.35 +34:59:41.3 -- not a known variable star
18:20:25.92 +36:19:43.6 -- not a known variable star
18:20:26.19 +35:05:09.8 -- not a known variable star
18:20:27.60 +35:35:25.4 -- not a known variable star
18:20:28.81 +36:08:37.9 -- not a known variable star
18:20:29.47 +35:43:37.3 -- not a known variable star
18:20:29.66 +35:41:56.9 -- not a known variable star
18:20:31.43 +36:08:32.3 -- not a known variable star
18:20:31.97 +35:43:18.5 -- not a known variable star
18:20:32.04 +35:15:23.7 -- not a known variable star
18:20:32.77 +35:25:08.5 -- not a known variable star
18:20:33.25 +35:49:00.3 -- not a known variable star
18:20:33.60 +35:43:43.7 -- not a known variable star
18:20:35.26 +35:55:01.5 -- not a known variable star
18:20:35.38 +36:10:32.0 -- not a known variable star
18:20:36.57 +36:17:20.7 -- not a known variable star
18:20:36.82 +35:07:35.9 -- not a known variable star
18:20:38.44 +35:53:23.9 -- not a known variable star
18:20:41.77 +35:36:27.3 -- not a known variable star
18:20:42.19 +36:10:54.9 -- not a known variable star
18:20:43.45 +35:46:58.4 -- not a known variable star
18:20:43.68 +35:44:26.9 -- not a known variable star
18:20:44.26 +36:10:32.8 -- not a known variable star
18:20:44.69 +34:59:48.5 -- not a known variable star
18:20:45.14 +35:07:21.2 -- not a known variable star
18:20:45.35 +35:12:54.8 -- not a known variable star
18:20:47.00 +36:05:52.4 -- not a known variable star
18:20:48.09 +35:43:33.7 -- not a known variable star
18:20:48.12 +36:06:49.9 -- a known variable star
18:20:49.28 +35:55:21.2 -- not a known variable star
18:20:50.39 +35:53:03.5 -- not a known variable star
18:20:51.13 +35:53:57.9 -- not a known variable star
18:20:51.60 +35:06:31.8 -- not a known variable star
18:20:52.29 +35:01:34.3 -- not a known variable star
18:20:52.60 +35:09:51.5 -- not a known variable star
18:20:52.79 +35:56:37.0 -- not a known variable star
18:20:54.04 +35:55:49.0 -- not a known variable star
18:20:55.49 +35:46:50.2 -- not a known variable star
18:20:55.53 +35:57:41.0 -- not a known variable star
18:20:55.56 +35:10:33.8 -- not a known variable star
18:20:55.76 +35:45:50.3 -- not a known variable star
18:20:56.48 +35:10:45.4 -- not a known variable star
18:20:56.60 +35:13:04.7 -- not a known variable star
18:20:58.03 +35:06:31.0 -- not a known variable star
18:20:58.35 +36:10:37.0 -- not a known variable star
18:20:58.88 +36:05:50.3 -- not a known variable star
18:20:59.23 +36:09:09.9 -- not a known variable star
18:21:02.14 +35:11:59.1 -- not a known variable star
18:21:02.95 +35:55:38.0 -- not a known variable star
18:21:05.44 +35:34:18.6 -- not a known variable star
18:21:05.80 +36:03:22.3 -- not a known variable star
18:21:05.85 +35:51:42.5 -- not a known variable star
18:21:06.43 +35:05:07.3 -- a known variable star
18:21:06.66 +36:16:57.2 -- not a known variable star
18:21:07.98 +35:46:37.9 -- not a known variable star
18:21:08.16 +36:00:06.7 -- not a known variable star
18:21:09.78 +36:08:39.4 -- not a known variable star
18:21:11.00 +35:13:38.5 -- not a known variable star
18:21:14.20 +35:06:38.9 -- not a known variable star
18:21:17.23 +35:50:46.1 -- not a known variable star
18:21:17.39 +35:03:52.7 -- not a known variable star
18:21:18.87 +35:03:38.1 -- not a known variable star
18:21:20.47 +35:35:19.5 -- not a known variable star
18:21:20.68 +35:00:44.7 -- not a known variable star
18:21:21.19 +35:18:41.3 -- not a known variable star
18:21:21.37 +36:11:25.2 -- not a known variable star
18:21:24.59 +35:06:19.7 -- not a known variable star
18:21:31.45 +36:04:17.8 -- not a known variable star
18:21:32.47 +35:05:01.3 -- not a known variable star
18:21:34.99 +35:37:40.3 -- not a known variable star
18:21:38.25 +35:00:00.4 -- not a known variable star
18:21:38.39 +35:22:32.0 -- not a known variable star
18:21:38.73 +35:06:39.7 -- not a known variable star
18:21:38.96 +35:14:57.1 -- not a known variable star
18:21:39.39 +35:36:42.5 -- not a known variable star
18:21:40.01 +35:09:46.6 -- not a known variable star
18:21:41.25 +35:02:37.6 -- not a known variable star
18:21:42.28 +35:45:08.3 -- not a known variable star
18:21:43.51 +34:53:21.6 -- not a known variable star
18:21:44.02 +35:28:26.2 -- not a known variable star
18:21:46.48 +35:02:24.0 -- a known variable star
18:21:53.41 +35:11:15.3 -- not a known variable star
18:21:54.62 +34:51:53.7 -- a known variable star
18:21:54.73 +34:56:11.3 -- not a known variable star
18:21:56.21 +36:31:39.2 -- not a known variable star
18:21:57.01 +35:59:21.1 -- not a known variable star
18:21:58.83 +35:07:13.8 -- a known variable star
18:21:59.21 +36:04:36.7 -- not a known variable star
18:22:02.51 +35:13:38.4 -- not a known variable star
18:22:03.95 +35:47:58.2 -- not a known variable star
18:22:04.90 +34:57:58.9 -- a known variable star
18:22:06.38 +35:07:35.9 -- not a known variable star
18:22:06.80 +35:57:17.6 -- not a known variable star
18:22:06.95 +35:10:40.0 -- not a known variable star
18:22:11.20 +35:39:36.5 -- not a known variable star
18:22:11.65 +35:45:27.2 -- not a known variable star
18:22:17.09 +36:00:29.1 -- not a known variable star
18:22:17.46 +36:03:34.7 -- not a known variable star
18:22:21.77 +34:54:00.4 -- not a known variable star
18:22:28.47 +35:30:41.5 -- not a known variable star
18:22:28.74 +35:48:07.7 -- not a known variable star
18:22:44.76 +35:34:27.0 -- not a known variable star
18:22:53.10 +35:46:21.5 -- not a known variable star
18:22:54.85 +36:00:21.0 -- not a known variable star
18:22:56.36 +35:56:58.7 -- not a known variable star
18:23:08.03 +35:49:54.8 -- not a known variable star
18:23:10.68 +35:53:25.6 -- not a known variable star
18:23:48.96 +35:48:39.9 -- not a known variable star
18:23:51.35 +35:49:26.9 -- not a known variable star
18:23:52.95 +37:06:52.9 -- not a known variable star
18:24:06.76 +37:13:19.9 -- not a known variable star
18:24:33.46 +37:22:21.6 -- not a known variable star
18:24:51.53 +36:33:42.8 -- not a known variable star
18:25:27.50 +37:16:23.3 -- not a known variable star
18:25:29.17 +36:32:12.6 -- not a known variable star
18:25:36.73 +37:24:42.1 -- not a known variable star
18:25:41.48 +37:36:35.3 -- not a known variable star
18:25:42.68 +39:17:45.6 -- not a known variable star
18:25:48.28 +36:48:27.2 -- not a known variable star
18:25:55.58 +37:02:24.6 -- not a known variable star
18:25:56.89 +37:04:27.0 -- not a known variable star
18:26:02.91 +36:30:46.2 -- not a known variable star
18:26:03.15 +37:37:41.7 -- not a known variable star
18:26:04.21 +37:03:38.3 -- not a known variable star
18:26:04.39 +37:34:52.4 -- not a known variable star
18:26:06.96 +37:14:57.3 -- not a known variable star
18:26:07.17 +37:28:48.5 -- not a known variable star
18:26:09.35 +36:30:32.5 -- not a known variable star
18:26:09.97 +36:58:52.6 -- not a known variable star
18:26:10.02 +37:25:31.9 -- not a known variable star
18:26:13.77 +36:59:13.5 -- a known variable star
18:26:15.52 +36:30:44.3 -- not a known variable star
18:26:19.58 +36:40:05.0 -- not a known variable star
18:26:22.68 +37:25:58.6 -- not a known variable star
18:26:24.92 +37:11:09.6 -- not a known variable star
18:26:25.54 +37:25:40.5 -- not a known variable star
18:26:30.95 +36:58:23.7 -- not a known variable star
18:26:33.88 +37:01:21.9 -- not a known variable star
18:26:34.05 +36:52:02.1 -- not a known variable star
18:26:35.10 +36:31:43.2 -- not a known variable star
18:26:36.99 +36:57:29.7 -- not a known variable star
18:26:38.99 +36:29:21.1 -- not a known variable star
18:26:40.54 +36:34:19.4 -- not a known variable star
18:26:43.33 +37:15:35.8 -- not a known variable star
18:26:43.57 +36:59:14.0 -- not a known variable star
18:26:45.08 +36:52:48.1 -- not a known variable star
18:26:48.51 +37:30:11.4 -- not a known variable star
18:26:49.82 +36:53:36.3 -- not a known variable star
18:26:50.38 +36:25:27.4 -- not a known variable star
18:26:53.88 +36:55:50.0 -- not a known variable star
18:26:55.22 +37:08:05.7 -- not a known variable star
18:26:56.02 +36:37:39.4 -- not a known variable star
18:26:57.73 +37:09:48.1 -- not a known variable star
18:26:58.78 +36:47:15.0 -- not a known variable star
18:27:02.28 +36:32:23.1 -- not a known variable star
18:27:15.54 +36:12:12.6 -- not a known variable star
18:27:19.20 +37:15:39.5 -- a known variable star
18:27:26.25 +36:27:37.9 -- not a known variable star
18:27:29.01 +36:11:44.6 -- not a known variable star
18:27:36.25 +36:59:42.3 -- not a known variable star
18:27:38.95 +36:52:32.1 -- not a known variable star
18:27:47.72 +36:09:51.1 -- not a known variable star
18:27:47.76 +36:34:36.4 -- not a known variable star
18:27:56.66 +36:23:24.0 -- not a known variable star
18:27:59.95 +36:49:13.0 -- not a known variable star
18:28:12.22 +36:17:47.5 -- not a known variable star
18:28:14.94 +36:18:47.9 -- not a known variable star
18:28:25.39 +37:15:31.4 -- not a known variable star
18:28:25.53 +36:15:34.4 -- not a known variable star
18:32:54.76 +39:03:22.7 -- not a known variable star
18:38:07.84 +37:38:16.8 -- not a known variable star
Found 301 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
326 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 326 (excluding asteroids and hot pixels, 301 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
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461239.75925507 -observatory V36
07:12:34.97 +17:30:53.1 Mercury (4.0mag)
10:44:02.44 +09:05:53.0 Venus (-4.2mag)
04:47:36.85 +22:18:15.9 Mars (1.3mag)
08:23:52.76 +19:48:13.8 Jupiter (-1.8mag)
00:56:31.56 +03:22:19.7 Saturn (0.7mag)
04:08:40.81 +20:48:56.2 Uranus (5.8mag)
00:16:55.65 +00:19:36.4 Neptune (7.7mag)
20:30:10.40 -23:21:29.0 Pluto (14.4mag)
11:06:49.96 +03:11:00.2 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jul 18 08:45 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461239.75925507:
08:23:49.79 +19:48:24.9 Io (6.0mag)
08:24:04.13 +19:47:30.1 Europa (6.3mag)
08:24:09.06 +19:47:09.6 Ganymede (5.6mag)
08:23:26.68 +19:49:54.8 Callisto (6.8mag)
08:22:03.58 +19:35:56.6 Himalia (15.7mag)
08:23:52.01 +19:48:17.7 Thebe (16.6mag)
08:21:24.60 +19:38:40.7 Elara (17.7mag)
08:27:38.54 +19:38:11.6 Pasiphae (17.9mag)
08:28:22.98 +19:54:30.8 Carme (19.0mag)
00:56:41.85 +03:22:26.9 Titan (8.5mag)
00:56:31.33 +03:22:29.8 Rhea (9.8mag)
00:55:57.05 +03:20:10.2 Iapetus (11.2mag)
00:56:18.41 +03:22:10.8 Hyperion (14.5mag)
00:56:21.70 +03:18:24.6 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 08:45 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.75925507:
17:58:54.72 -31:05:31.5 JWST
16:12:08.56 +50:00:28.0 Chandra
22:02:25.71 +54:09:17.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 08:45 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.75925507 -observatory V36
02:47:18.76 +15:20:20.1 17.8mag P/1996 R2 (Lagerkvist)
18:12:09.77 -34:32:35.2 13.8mag P/2010 H2 (Vales)
06:33:33.64 -68:17:05.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:30.25 +32:35:04.8 17.6mag C/2017 K2 (PANSTARRS)
02:28:07.43 +21:14:22.8 15.8mag P/2021 N1 (ZTF)
22:54:31.28 +32:13:30.0 17.3mag C/2022 E2 (ATLAS)
06:21:19.41 +26:50:49.5 16.7mag C/2022 N2 (PANSTARRS)
10:02:28.45 +29:25:28.3 16.9mag C/2022 QE78 (ATLAS)
09:14:52.97 +05:07:58.7 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.76 -11:35:05.4 17.8mag P/2023 B1 (PANSTARRS)
21:39:17.29 +67:29:04.9 17.9mag C/2023 H5 (Lemmon)
16:16:12.54 -10:53:44.4 14.0mag C/2023 R1 (PANSTARRS)
08:14:36.12 +66:08:55.2 17.9mag C/2024 A1 (ATLAS)
07:43:01.34 +30:23:38.5 14.8mag C/2024 E1 (Wierzchos)
15:12:48.51 +15:30:01.3 17.6mag C/2024 G6 (ATLAS)
19:31:00.48 +40:48:48.8 13.7mag C/2024 J3 (ATLAS)
21:38:53.87 +47:07:52.0 17.8mag C/2024 R4 (PANSTARRS)
04:57:00.90 -13:28:09.5 15.7mag C/2024 T5 (ATLAS)
06:41:00.18 +27:44:52.9 18.0mag C/2025 J1 (Borisov)
07:19:39.13 -13:38:02.5 16.9mag C/2025 R3 (PANSTARRS)
10:05:29.11 +22:04:42.1 17.5mag C/2025 V2 (Rankin)
12:47:31.36 +03:34:30.7 17.0mag C/2025 Y1 (ATLAS)
16:31:04.81 +79:07:46.5 17.2mag C/2026 A2 (Bok)
02:54:06.12 +45:33:53.8 16.8mag C/2026 B2 (Sun-Gao)
11:30:45.64 +05:51:49.4 17.0mag A/2026 E1
21:31:08.18 -18:06:43.0 7.1mag 10P/Tempel
11:17:18.20 -02:14:39.1 16.2mag 29P/Schwassmann-Wachmann
04:11:26.60 +30:23:48.5 17.9mag 47P/Ashbrook-Jackson
10:24:33.45 +11:28:35.6 17.1mag 63P/Wild
00:51:23.36 -05:02:47.8 15.5mag 65P/Gunn
04:46:27.41 +20:31:33.8 13.7mag 78P/Gehrels
02:34:39.42 +11:38:37.6 16.4mag 88P/Howell
06:58:46.01 +29:59:02.7 15.8mag 93P/Lovas
04:46:51.89 +31:19:48.5 16.7mag 114P/Wiseman-Skiff
08:28:00.30 +29:46:04.2 15.2mag 123P/West-Hartley
11:02:59.14 -02:00:54.5 16.9mag 124P/Mrkos
05:04:21.89 +21:00:36.4 16.2mag 128P/Shoemaker-Holt
05:51:03.81 +19:36:48.5 17.8mag 131P/Mueller
07:41:41.84 +15:15:37.1 16.5mag 141P-D/Machholz
03:20:17.89 -20:45:05.9 15.1mag 161P/Hartley-IRAS
06:01:36.10 +35:29:41.6 15.5mag 162P/SidingSpring
18:39:21.39 +20:30:15.0 14.0mag 169P/NEAT
01:59:33.32 +08:24:24.1 17.6mag 220P/McNaught
16:35:32.55 -08:44:35.7 17.2mag 235P/LINEAR
09:01:49.29 +32:32:33.9 18.0mag 240P/NEAT
20:37:57.51 -51:08:31.6 17.8mag 259P/Garradd
02:21:35.35 +15:47:13.3 15.6mag 260P/McNaught
06:01:19.49 +37:23:08.3 17.3mag 295P/LINEAR
15:06:33.42 +05:19:33.4 17.6mag 391P/Kowalski
08:41:44.52 +19:20:48.5 17.9mag 450P/LONEOS
08:04:06.78 +38:33:10.9 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 08:45 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -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
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
-rw-r--r-- 1 apache apache 5.6K Jul 18 08:45 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 18 08:45 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:40:11.159 -09:00:57.92 AT 2026swa 2026-06-27.33 23.1049
21:35:24.753 -14:51:35.01 AT 2026svz 2026-06-27.33 22.2271
20:31:55.032 -25:17:26.05 AT 2026svy 2026-06-27.32 22.425
23:12:03.386 -07:08:51.16 AT 2026svx 2026-06-27.43 22.3341
21:38:52.469 -09:12:08.16 AT 2026svw 2026-06-27.33 20.826
21:24:07.399 -08:10:48.32 AT 2026svv 2026-06-27.34 22.9964
20:42:22.608 -20:56:09.99 AT 2026svu 2026-06-27.32 22.8033
22:49:29.419 -09:52:21.90 AT 2026svt 2026-06-27.41 23.2399
23:08:56.975 -10:56:50.31 AT 2026svs 2026-06-27.42 23.0562
23:03:48.038 -10:42:20.17 AT 2026svr 2026-06-27.42 23.1156
21:05:20.116 -12:39:02.09 AT 2026svq 2026-06-27.30 22.4649
04:03:37.997 -49:14:19.96 AT 2026svp 2026-06-26.43 23.1019
21:42:26.450 -12:30:39.78 AT 2026svo 2026-06-26.41 23.1202
22:23:57.549 -05:26:28.43 AT 2026svn 2026-06-26.40 23.0846
21:59:30.646 -08:36:23.43 AT 2026svm 2026-06-26.41 23.0458
00:40:45.913 -42:36:08.06 AT 2026svl 2026-06-26.42 23.627
22:01:49.708 -02:28:35.92 AT 2026svk 2026-06-26.41 22.3804
22:26:37.642 -04:12:59.57 AT 2026svj 2026-06-26.40 22.8575
21:46:45.471 -13:57:34.56 AT 2026svi 2026-06-26.41 22.7499
21:42:08.217 -14:29:27.43 AT 2026svh 2026-06-26.41 23.2705
-rw-r--r-- 1 apache apache 89K Jul 18 08:45 tns_transients_list.txt
