This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.99 21:31:28.72 +39:48:09.6
86.42260 -8.49335 galactic Cyg Second-epoch detections are separated by 1.8" and 7.4 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 | 21:31:28.72 +39:48:09.6 (user input) | T | P | (position from user input) J-Ks=0.705+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:28.72 +39:48:09.6: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:28.72 +39:48:09.6: 14.02 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 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 05 17.4465 2461177.9465 11.66 22:23:52.17 +39:48:15.6
94.44650 -14.76830 galactic Lac Second-epoch detections are separated by 3.4" and 6.5 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 | 22:23:52.17 +39:48:15.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:52.17 +39:48:15.6: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:52.17 +39:48:15.6: 14.18 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.60 22:17:40.49 +40:49:15.2
94.02581 -13.26459 galactic Lac Second-epoch detections are separated by 2.8" and 7.0 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 | 22:17:40.49 +40:49:15.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:40.49 +40:49:15.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:40.49 +40:49:15.2: 14.18 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.78 21:16:59.17 +37:32:52.5
82.79055 -8.08912 galactic Cyg Second-epoch detections are separated by 3.4" and 8.3 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 J319.2382+37.5501 | 21:16:59.17 +37:32:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:59.17 +37:32:52.5: 13.01 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:59.17 +37:32:52.5: 13.86 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.2382+37.5501,2461177.9465,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.2382+37.5501 20260517.4465 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 05 17.4465 2461177.9465 11.48 22:22:14.11 +41:40:45.7
95.24905 -13.03490 galactic Lac Second-epoch detections are separated by 4.3" and 6.2 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 J335.5601+41.6764 | 22:22:14.11 +41:40:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.447+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:14.11 +41:40:45.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:14.11 +41:40:45.7: 13.92 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.5601+41.6764,2461177.9465,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.5601+41.6764 20260517.4465 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.52 21:54:37.12 +36:25:58.5
87.60698 -14.03392 galactic Peg Second-epoch detections are separated by 3.8" and 6.9 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 | 21:54:37.12 +36:25:58.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:37.12 +36:25:58.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:37.12 +36:25:58.5: 13.95 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.37 21:12:16.07 +34:09:55.3
79.62823 -9.69986 galactic Cyg Second-epoch detections are separated by 5.1" and 8.6 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 | 21:12:16.07 +34:09:55.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:16.07 +34:09:55.3: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:16.07 +34:09:55.3: 13.53 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.52 22:01:22.35 +40:55:07.5
91.54115 -11.36349 galactic Lac Second-epoch detections are separated by 2.5" and 7.5 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 J330.3389+40.9153 | 22:01:22.35 +40:55:07.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.35 +40:55:07.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:22.35 +40:55:07.5: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 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
ATO J330.3389+40.9153,2461177.9465,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3389+40.9153 20260517.4465 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.53 21:21:02.46 +42:07:14.1
86.63829 -5.45892 galactic Cyg Second-epoch detections are separated by 2.4" and 7.4 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 J320.2455+42.1181 | 21:21:02.46 +42:07:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.046+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:02.46 +42:07:14.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:02.46 +42:07:14.1: 13.52 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.2455+42.1181,2461177.9465,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.2455+42.1181 20260517.4465 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.38 22:24:29.08 +33:18:07.3
90.73759 -20.22682 galactic Peg Second-epoch detections are separated by 2.0" and 7.4 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 | 22:24:29.08 +33:18:07.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:29.08 +33:18:07.3: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:29.08 +33:18:07.3: 14.16 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.26 21:47:22.88 +33:57:51.4
84.78769 -14.94427 galactic Cyg Second-epoch detections are separated by 4.2" and 7.8 pix
The object was found in VSX 5" ZTF J214722.97+335756.5
Type: RS
# Max. Min./Amp. JD0 Period
13.922 r Y 0.046 r 2458266.85650 0.626117300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:22.88 +33:57:51.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:22.88 +33:57:51.4: 13.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J214722.97+335756.5,2461177.9465,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214722.97+335756.5 20260517.4465 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.37 21:57:39.28 +41:47:18.1
91.52943 -10.24866 galactic Lac Second-epoch detections are separated by 1.3" and 7.3 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 J329.4174+41.7911 | 21:57:39.28 +41:47:18.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.534+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:39.28 +41:47:18.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.28 +41:47:18.1: 13.43 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.43 +/- 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
ATO J329.4174+41.7911,2461177.9465,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4174+41.7911 20260517.4465 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.09 21:14:24.68 +33:06:52.2
79.14849 -10.73930 galactic Cyg Second-epoch detections are separated by 1.6" and 7.9 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 | 21:14:24.68 +33:06:52.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:24.68 +33:06:52.2: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:24.68 +33:06:52.2: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.23 +/- 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
target,2461177.9465,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 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 05 17.4465 2461177.9465 11.04 22:20:17.38 +34:47:25.5
90.88267 -18.50880 galactic Peg Second-epoch detections are separated by 2.7" and 6.9 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 J335.0723+34.7873 | 22:20:17.38 +34:47:25.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.349+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:17.38 +34:47:25.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:17.38 +34:47:25.5: 13.82 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.0723+34.7873,2461177.9465,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.0723+34.7873 20260517.4465 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.96 21:11:40.23 +34:59:54.3
80.16697 -9.04675 galactic Cyg Second-epoch detections are separated by 4.6" and 7.9 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 J317.9134+34.9984 | 21:11:40.23 +34:59:54.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:40.23 +34:59:54.3: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:40.23 +34:59:54.3: 13.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.9134+34.9984,2461177.9465,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.9134+34.9984 20260517.4465 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.11 21:48:47.02 +40:08:13.0
89.14850 -10.46165 galactic Cyg Second-epoch detections are separated by 0.6" and 7.2 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 J327.1964+40.1375 | 21:48:43.45 +40:08:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:47.02 +40:08:13.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:47.02 +40:08:13.0: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 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
ATO J327.1964+40.1375,2461177.9465,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1964+40.1375 20260517.4465 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.15 21:12:49.69 +41:23:26.1
85.04290 -4.86388 galactic Cyg Second-epoch detections are separated by 1.9" and 8.1 pix
The object was found in VSX 3" V1234 Cyg
Type: M:
# Max. Min./Amp. JD0 Period
16.500 B < 18.000 B 2442723.00000 222.000000000000 M7-M9
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:49.69 +41:23:26.1: 12.19 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:49.69 +41:23:26.1: 14.01 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1234 Cyg,2461177.9465,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1234 Cyg 20260517.4465 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.95 21:33:38.23 +37:37:16.6
85.21018 -10.36560 galactic Cyg Second-epoch detections are separated by 0.9" and 7.7 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 | 21:33:38.23 +37:37:16.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:38.23 +37:37:16.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:38.23 +37:37:16.6: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 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,2461177.9465,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.08 21:33:10.78 +39:46:10.6
86.63969 -8.74195 galactic Cyg Second-epoch detections are separated by 2.1" and 7.6 pix
The object was found in VSX 9" NSVS 5918143
Type: SR
# Max. Min./Amp. JD0 Period
13.055 r Y 0.513 r 2458273.93180 220.436025900000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:10.78 +39:46:10.6: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:10.78 +39:46:10.6: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 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
NSVS 5918143,2461177.9465,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5918143 20260517.4465 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.86 22:27:29.73 +41:09:13.6
95.80333 -14.01388 galactic Lac Second-epoch detections are separated by 2.6" and 7.3 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 | 22:27:29.73 +41:09:13.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:29.73 +41:09:13.6: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:29.73 +41:09:13.6: 13.41 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.62 21:28:08.25 +36:39:03.2
83.72352 -10.30274 galactic Cyg Second-epoch detections are separated by 1.8" and 7.5 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 J322.0157+36.6584 | 21:28:06.52 +36:38:58.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.021+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:08.25 +36:39:03.2: 12.39 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:08.25 +36:39:03.2: 12.76 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.75 +/- 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
ATO J322.0157+36.6584,2461177.9465,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0157+36.6584 20260517.4465 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.76 21:20:25.20 +37:31:57.8
83.25686 -8.58983 galactic Cyg Second-epoch detections are separated by 0.4" and 7.8 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 J320.1010+37.5280 | 21:20:25.20 +37:31:57.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.648+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:25.20 +37:31:57.8: 11.50 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:25.20 +37:31:57.8: 12.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.52 +/- 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 J320.1010+37.5280,2461177.9465,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.1010+37.5280 20260517.4465 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.52 22:05:08.02 +36:40:55.1
89.46977 -15.16131 galactic Lac Second-epoch detections are separated by 2.3" and 7.2 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 | 22:05:08.02 +36:40:55.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:08.02 +36:40:55.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:08.02 +36:40:55.1: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 8.06 22:01:07.90 +39:15:18.8
90.45759 -12.64653 galactic Lac Second-epoch detections are separated by 0.2" and 7.2 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 | HIP 108695 | 22:01:06.72 +39:14:45.4 (Gaia DR3) | VAR (local) | 2.479670000000 (local) | Gaia3var=VARIABLE SpType: A0 1947IzKry...1...44S HD 209260 J-Ks=0.278+/-0.032 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:07.90 +39:15:18.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:07.90 +39:15:18.8: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.26 +/- 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
HIP 108695,2461177.9465,8.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HIP 108695 20260517.4465 8.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.35 21:31:14.85 +38:46:29.2
85.67186 -9.20630 galactic Cyg Second-epoch detections are separated by 1.2" and 7.6 pix
The object was found in VSX 4" V2072 Cyg
Type: M
# Max. Min./Amp. JD0 Period
10.400 V 17.900 V 2451388.00000 317.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:14.85 +38:46:29.2: 12.57 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:14.85 +38:46:29.2: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 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
V2072 Cyg,2461177.9465,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2072 Cyg 20260517.4465 9.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.36 22:29:53.29 +41:25:59.8
96.34879 -14.01825 galactic Lac Second-epoch detections are separated by 0.8" and 7.0 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 J337.4722+41.4238 | 22:29:53.38 +41:26:01.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.062+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:53.29 +41:25:59.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:53.29 +41:25:59.8: 12.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 J337.4722+41.4238,2461177.9465,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J337.4722+41.4238 20260517.4465 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.88 21:15:49.53 +38:27:47.2
83.30040 -7.29252 galactic Cyg Second-epoch detections are separated by 1.8" and 8.1 pix
The object was found in VSX 1" ASASSN-V J211549.62+382747.5
Type: SR
# Max. Min./Amp. JD0 Period
13.810 V 14.300 V 2457871.10000 76.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:49.53 +38:27:47.2: 11.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:49.53 +38:27:47.2: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 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
ASASSN-V J211549.62+382747.5,2461177.9465,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211549.62+382747.5 20260517.4465 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.40 21:21:47.75 +35:29:49.3
81.97386 -10.20797 galactic Cyg Second-epoch detections are separated by 1.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1855474216027817600 | 21:21:45.57 +35:29:44.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:47.75 +35:29:49.3: 11.20 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:47.75 +35:29:49.3: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855474216027817600,2461177.9465,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1855474216027817600 20260517.4465 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.49 21:17:37.36 +36:35:15.1
82.17653 -8.84385 galactic Cyg Second-epoch detections are separated by 1.0" and 8.0 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 | 21:17:37.36 +36:35:15.1 (user input) | T | P | (position from user input) J-Ks=0.582+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:37.36 +36:35:15.1: 11.70 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:37.36 +36:35:15.1: 12.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.57 +/- 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,2461177.9465,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.54 22:20:55.87 +41:36:25.0
94.99988 -12.95977 galactic Lac Second-epoch detections are separated by 1.5" and 6.7 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 J335.2412+41.5961 | 22:20:55.87 +41:36:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:55.87 +41:36:25.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:55.87 +41:36:25.0: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
ATO J335.2412+41.5961,2461177.9465,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.2412+41.5961 20260517.4465 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.62 21:26:25.15 +35:51:23.8
82.90483 -10.62324 galactic Cyg Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.6060+35.8609 | 21:26:25.15 +35:51:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.349+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:25.15 +35:51:23.8: 11.61 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:25.15 +35:51:23.8: 12.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 J321.6060+35.8609,2461177.9465,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.6060+35.8609 20260517.4465 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.75 21:17:44.37 +33:45:12.6
80.10624 -10.81147 galactic Cyg Second-epoch detections are separated by 1.4" and 8.2 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 | 21:17:44.37 +33:45:12.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:44.37 +33:45:12.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:44.37 +33:45:12.6: 13.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.04 +/- 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
target,2461177.9465,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.88 22:02:13.83 +41:47:07.6
92.21108 -10.77627 galactic Lac Second-epoch detections are separated by 1.2" and 7.2 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 J330.5515+41.7805 | 22:02:12.37 +41:46:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.975+/-0.036 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:13.83 +41:47:07.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:13.83 +41:47:07.6: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 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
ATO J330.5515+41.7805,2461177.9465,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5515+41.7805 20260517.4465 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.81 22:07:05.43 +37:55:15.5
90.56834 -14.41410 galactic Lac Second-epoch detections are separated by 1.4" and 7.3 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 J331.7704+37.9239 | 22:07:05.43 +37:55:15.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:05.43 +37:55:15.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:05.43 +37:55:15.5: 13.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.40 +/- 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
ATO J331.7704+37.9239,2461177.9465,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.7704+37.9239 20260517.4465 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.86 22:26:44.90 +40:34:43.6
95.36003 -14.42121 galactic Lac Second-epoch detections are separated by 0.8" and 6.9 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 | 22:26:44.90 +40:34:43.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:44.90 +40:34:43.6: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:44.90 +40:34:43.6: 13.97 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.90 21:24:39.60 +36:58:44.7
83.45705 -9.57939 galactic Cyg Second-epoch detections are separated by 4.2" and 7.5 pix
The object was found in VSX22" Gaia DR3 1963742408760031616
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.410 G 14.440 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:39.60 +36:58:44.7: 11.73 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:39.60 +36:58:44.7: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 1963742408760031616,2461177.9465,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963742408760031616 20260517.4465 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.82 22:07:49.41 +33:25:38.1
87.84392 -18.07156 galactic Peg Second-epoch detections are separated by 2.0" and 7.7 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 J331.9469+33.4302 | 22:07:49.41 +33:25:38.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:49.41 +33:25:38.1: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:49.41 +33:25:38.1: 13.68 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9469+33.4302,2461177.9465,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9469+33.4302 20260517.4465 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.90 21:58:07.66 +38:56:39.7
89.79179 -12.52796 galactic Lac Second-epoch detections are separated by 1.9" and 7.5 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 | 21:58:07.66 +38:56:39.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:07.66 +38:56:39.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:07.66 +38:56:39.7: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.50 +/- 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
target,2461177.9465,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.01 21:35:16.75 +37:59:46.9
85.71155 -10.31470 galactic Cyg Second-epoch detections are separated by 3.1" and 8.0 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 | 21:35:16.75 +37:59:46.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:16.75 +37:59:46.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:16.75 +37:59:46.9: 13.22 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 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,2461177.9465,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.03 21:17:23.18 +41:27:44.6
85.68713 -5.43266 galactic Cyg Second-epoch detections are separated by 1.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.3531+41.4500 | 21:17:25.55 +41:27:31.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.840+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:23.18 +41:27:44.6: 12.98 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:23.18 +41:27:44.6: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 J319.3531+41.4500,2461177.9465,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.3531+41.4500 20260517.4465 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.16 21:29:07.94 +42:01:02.3
87.64198 -6.58549 galactic Cyg Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 4" Gaia DR3 1967190545946435712
Type: ROT
# Max. Min./Amp. JD0 Period
14.270 G 14.290 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:07.94 +42:01:02.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:07.94 +42:01:02.3: 13.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1967190545946435712,2461177.9465,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967190545946435712 20260517.4465 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.97 21:57:40.54 +37:18:47.0
88.66913 -13.74198 galactic Cyg Second-epoch detections are separated by 2.1" and 7.0 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 J329.4294+37.3037 | 21:57:40.54 +37:18:47.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:40.54 +37:18:47.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:40.54 +37:18:47.0: 13.47 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 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
ATO J329.4294+37.3037,2461177.9465,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4294+37.3037 20260517.4465 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.93 21:15:42.90 +33:53:34.2
79.91708 -10.40942 galactic Cyg Second-epoch detections are separated by 1.1" and 8.1 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 J318.9171+33.8998 | 21:15:42.90 +33:53:34.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:42.90 +33:53:34.2: 12.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:42.90 +33:53:34.2: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.87 +/- 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
ATO J318.9171+33.8998,2461177.9465,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.9171+33.8998 20260517.4465 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.01 21:20:52.04 +38:17:39.3
83.86991 -8.12098 galactic Cyg Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1964847898984320640 | 21:20:48.66 +38:17:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/- (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:52.04 +38:17:39.3: 11.89 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:52.04 +38:17:39.3: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 1964847898984320640,2461177.9465,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964847898984320640 20260517.4465 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.98 21:48:37.93 +41:48:10.0
90.21891 -9.17192 galactic Cyg Second-epoch detections are separated by 4.5" and 6.5 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 J327.1580+41.8073 | 21:48:37.93 +41:48:10.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:37.93 +41:48:10.0: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:37.93 +41:48:10.0: 13.47 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 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
ATO J327.1580+41.8073,2461177.9465,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1580+41.8073 20260517.4465 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.13 21:18:35.07 +40:16:41.5
84.99081 -6.41954 galactic Cyg Second-epoch detections are separated by 1.4" and 7.8 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 J319.6471+40.2846 | 21:18:33.06 +40:16:53.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:35.07 +40:16:41.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:35.07 +40:16:41.5: 13.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.02 +/- 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
ATO J319.6471+40.2846,2461177.9465,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.6471+40.2846 20260517.4465 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.99 21:16:29.73 +36:57:21.7
82.28921 -8.42632 galactic Cyg Second-epoch detections are separated by 2.4" and 7.8 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 J319.1111+36.9565 | 21:16:26.75 +36:57:48.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:29.73 +36:57:21.7: 12.12 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:29.73 +36:57:21.7: 13.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.1111+36.9565,2461177.9465,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.1111+36.9565 20260517.4465 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.08 21:14:44.85 +38:12:02.9
82.96183 -7.31930 galactic Cyg Second-epoch detections are separated by 2.9" and 7.7 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 J318.6921+38.2089 | 21:14:44.85 +38:12:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:44.85 +38:12:02.9: 12.77 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:44.85 +38:12:02.9: 13.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J318.6921+38.2089,2461177.9465,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.6921+38.2089 20260517.4465 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.10 22:06:31.85 +34:33:34.9
88.35020 -17.01269 galactic Peg Second-epoch detections are separated by 4.6" and 7.9 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 | 22:06:31.85 +34:33:34.9 (user input) | T | P | (position from user input) J-Ks=0.631+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:31.85 +34:33:34.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:31.85 +34:33:34.9: 14.25 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.13 21:34:48.95 +41:16:17.1
87.90519 -7.85652 galactic Cyg Second-epoch detections are separated by 2.7" and 7.0 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 J323.7026+41.2683 | 21:34:48.95 +41:16:17.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.422+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:48.95 +41:16:17.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:48.95 +41:16:17.1: 13.43 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.43 +/- 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
ATO J323.7026+41.2683,2461177.9465,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.7026+41.2683 20260517.4465 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.19 22:17:36.78 +42:32:37.0
95.01675 -11.83897 galactic Lac Second-epoch detections are separated by 1.3" and 7.1 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 J334.4057+42.5309 | 22:17:36.78 +42:32:37.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.809+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:36.78 +42:32:37.0: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:36.78 +42:32:37.0: 13.95 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.4057+42.5309,2461177.9465,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.4057+42.5309 20260517.4465 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.09 22:06:46.45 +39:39:12.0
91.59213 -12.99438 galactic Lac Second-epoch detections are separated by 3.0" and 6.6 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 | 22:06:46.45 +39:39:12.0 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:46.45 +39:39:12.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:46.45 +39:39:12.0: 13.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 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 05 17.4465 2461177.9465 11.10 21:42:06.01 +36:50:53.5
85.93721 -12.07627 galactic Cyg Second-epoch detections are separated by 0.8" and 7.4 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 J325.5190+36.8572 | 21:42:02.55 +36:51:12.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:06.01 +36:50:53.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:06.01 +36:50:53.5: 13.46 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 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
ATO J325.5190+36.8572,2461177.9465,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5190+36.8572 20260517.4465 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.03 22:20:30.92 +33:33:33.5
90.17229 -19.54167 galactic Peg Second-epoch detections are separated by 2.4" and 7.5 pix
The object was found in VSX 3" Gaia DR3 1905073086772697088
Type: ROT
# Max. Min./Amp. JD0 Period
13.480 G 13.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:30.92 +33:33:33.5: 13.06 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:30.92 +33:33:33.5: 14.34 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1905073086772697088,2461177.9465,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905073086772697088 20260517.4465 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.20 21:10:36.26 +40:19:47.7
83.97628 -5.27985 galactic Cyg Second-epoch detections are separated by 0.4" and 7.8 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 | 21:10:36.26 +40:19:47.7 (user input) | T | P | (position from user input) J-Ks=0.839+/-0.028 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:36.26 +40:19:47.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:36.26 +40:19:47.7: 13.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.19 22:26:17.79 +40:38:19.1
95.31924 -14.32438 galactic Lac Second-epoch detections are separated by 3.2" and 7.4 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 | 22:26:17.79 +40:38:19.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:17.79 +40:38:19.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:17.79 +40:38:19.1: 14.36 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.30 22:15:17.67 +39:47:52.8
93.04043 -13.84301 galactic Lac Second-epoch detections are separated by 2.2" and 7.4 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 | 22:15:17.67 +39:47:52.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:15:17.67 +39:47:52.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:15:17.67 +39:47:52.8: 14.45 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.23 22:03:59.71 +39:46:37.0
91.23240 -12.57269 galactic Lac Second-epoch detections are separated by 3.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956551877588448768 | 22:03:57.02 +39:46:05.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:59.71 +39:46:37.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:59.71 +39:46:37.0: 13.74 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956551877588448768,2461177.9465,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956551877588448768 20260517.4465 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.35 21:29:05.00 +40:27:03.4
86.54136 -7.70844 galactic Cyg Second-epoch detections are separated by 3.2" and 7.7 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 J322.2754+40.4518 | 21:29:05.00 +40:27:03.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:05.00 +40:27:03.4: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:05.00 +40:27:03.4: 13.56 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.2754+40.4518,2461177.9465,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.2754+40.4518 20260517.4465 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.24 22:14:09.55 +38:28:25.4
92.06230 -14.79379 galactic Lac Second-epoch detections are separated by 3.0" and 7.6 pix
The object was found in VSX 7" Gaia DR3 1955341212206396160
Type: ROT
# Max. Min./Amp. JD0 Period
13.690 G 13.750 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:14:09.55 +38:28:25.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:14:09.55 +38:28:25.4: 13.77 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955341212206396160,2461177.9465,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955341212206396160 20260517.4465 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.28 21:25:05.40 +37:46:26.3
84.08795 -9.07783 galactic Cyg Second-epoch detections are separated by 0.8" and 7.8 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 J321.2679+37.7763 | 21:25:05.40 +37:46:26.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.265+/-0.076 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:05.40 +37:46:26.3: 12.33 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:05.40 +37:46:26.3: 13.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.02 +/- 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
ATO J321.2679+37.7763,2461177.9465,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.2679+37.7763 20260517.4465 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.36 21:27:59.53 +37:32:20.0
84.33432 -9.64889 galactic Cyg Second-epoch detections are separated by 3.7" and 7.1 pix
The object was found in VSX25" Gaia DR3 1964152938913010560
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.810 G 12.840 G 0.069962500000 A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:59.53 +37:32:20.0: 13.04 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:59.53 +37:32:20.0: 13.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1964152938913010560,2461177.9465,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964152938913010560 20260517.4465 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.23 21:44:49.60 +36:56:52.9
86.42131 -12.36478 galactic Cyg Second-epoch detections are separated by 1.1" and 7.6 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 | 21:44:49.60 +36:56:52.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:49.60 +36:56:52.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:49.60 +36:56:52.9: 14.02 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.37 21:42:23.21 +40:36:52.9
88.53151 -9.30278 galactic Cyg Second-epoch detections are separated by 1.0" and 7.3 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 J325.5857+40.6170 | 21:42:23.21 +40:36:52.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:23.21 +40:36:52.9: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:23.21 +40:36:52.9: 13.77 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5857+40.6170,2461177.9465,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5857+40.6170 20260517.4465 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.27 22:04:58.72 +32:49:10.1
86.95604 -18.18174 galactic Peg Second-epoch detections are separated by 1.9" and 7.4 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 | 22:04:58.72 +32:49:10.1 (user input) | T | P | (position from user input) J-Ks=0.652+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:58.72 +32:49:10.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:58.72 +32:49:10.1: 13.80 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.34 22:01:13.37 +38:32:59.7
90.02492 -13.21216 galactic Lac Second-epoch detections are separated by 1.8" and 7.0 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 J330.2962+38.5586 | 22:01:13.37 +38:32:59.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.341+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:13.37 +38:32:59.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:13.37 +38:32:59.7: 13.73 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2962+38.5586,2461177.9465,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2962+38.5586 20260517.4465 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.52 21:14:48.61 +37:08:04.4
82.18705 -8.05925 galactic Cyg Second-epoch detections are separated by 2.0" and 7.8 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 | 21:14:48.61 +37:08:04.4 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:48.61 +37:08:04.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:48.61 +37:08:04.4: 13.90 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.56 21:43:31.98 +38:44:13.9
87.43612 -10.85539 galactic Cyg Second-epoch detections are separated by 1.1" and 7.2 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 1953638957749125248 | 21:43:30.75 +38:43:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:31.98 +38:44:13.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:31.98 +38:44:13.9: 13.90 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953638957749125248,2461177.9465,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953638957749125248 20260517.4465 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.41 22:21:21.30 +41:17:35.5
94.88808 -13.26455 galactic Lac Second-epoch detections are separated by 0.7" and 7.0 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 J335.3499+41.2971 | 22:21:21.30 +41:17:35.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:21.30 +41:17:35.5: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:21.30 +41:17:35.5: 13.90 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.3499+41.2971,2461177.9465,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.3499+41.2971 20260517.4465 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.66 22:09:11.47 +36:46:04.4
90.19429 -15.58601 galactic Lac Second-epoch detections are separated by 3.9" and 7.1 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 J332.2936+36.7689 | 22:09:11.47 +36:46:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:11.47 +36:46:04.4: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:11.47 +36:46:04.4: 14.67 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2936+36.7689,2461177.9465,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2936+36.7689 20260517.4465 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 11.93 21:24:42.34 +38:26:37.6
84.51243 -8.55018 galactic Cyg Second-epoch detections are separated by 2.0" and 7.7 pix
The object was found in VSX 3" ASASSN-V J212442.51+382640.2
Type: M
# Max. Min./Amp. JD0 Period
20.450 g Y 4.379 g 2458324.51660 375.299483000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:42.34 +38:26:37.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:42.34 +38:26:37.6: 15.22 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212442.51+382640.2,2461177.9465,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212442.51+382640.2 20260517.4465 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 05 17.4465 2461177.9465 11.78 21:27:07.29 +35:14:56.3
82.57100 -11.15444 galactic Cyg Second-epoch detections are separated by 4.2" and 7.7 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 | 21:27:07.29 +35:14:56.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:07.29 +35:14:56.3: 12.44 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:07.29 +35:14:56.3: 14.30 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 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 05 17.4465 2461177.9465 11.79 22:02:04.62 +37:45:26.7
89.65695 -13.93901 galactic Lac Second-epoch detections are separated by 1.6" and 7.5 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 | 22:02:04.62 +37:45:26.7 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:04.62 +37:45:26.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:04.62 +37:45:26.7: 14.34 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.23 22:28:16.88 +41:56:37.5
96.36770 -13.42645 galactic Lac Second-epoch detections are separated by 1.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1957578134253911808 | 22:28:16.65 +41:56:39.2 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:16.88 +41:56:37.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:16.88 +41:56:37.5: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1957578134253911808,2461177.9465,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1957578134253911808 20260517.4465 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.16 22:24:47.79 +41:23:33.9
95.49834 -13.53792 galactic Lac Second-epoch detections are separated by 0.2" and 6.8 pix
The object was found in VSX12" Gaia DR3 1957496181979308928
Type: ROT
# Max. Min./Amp. JD0 Period
17.560 G 17.680 G 1.961320000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:47.79 +41:23:33.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:47.79 +41:23:33.9: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 1957496181979308928,2461177.9465,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1957496181979308928 20260517.4465 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.41 22:25:18.24 +34:10:33.3
91.41211 -19.60192 galactic Peg Second-epoch detections are separated by 0.3" and 7.3 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 1902579875437130624 | 22:25:18.29 +34:10:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.212+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:18.24 +34:10:33.3: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:18.24 +34:10:33.3: 12.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.71 +/- 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 1902579875437130624,2461177.9465,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902579875437130624 20260517.4465 9.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.61 22:25:05.70 +39:23:43.0
94.41702 -15.23973 galactic Lac Second-epoch detections are separated by 1.3" and 6.9 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 | 22:25:05.70 +39:23:43.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:05.70 +39:23:43.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:05.70 +39:23:43.0: 13.57 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.62 21:28:06.80 +39:56:16.2
86.04686 -7.94844 galactic Cyg Second-epoch detections are separated by 0.3" and 7.5 pix
The object was found in VSX 2" V0837 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.800 B 17.100 B 2443192.00000 292.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:06.80 +39:56:16.2: 12.99 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:06.80 +39:56:16.2: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0837 Cyg,2461177.9465,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0837 Cyg 20260517.4465 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.38 21:13:42.11 +34:07:20.2
79.79977 -9.94750 galactic Cyg Second-epoch detections are separated by 0.7" and 8.1 pix
The object was found in VSX 6" ASASSN-V J211341.76+340716.4
Type: SR
# Max. Min./Amp. JD0 Period
14.320 g Y 0.300 g 2459493.80000 52.710000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:42.11 +34:07:20.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:42.11 +34:07:20.2: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211341.76+340716.4,2461177.9465,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211341.76+340716.4 20260517.4465 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.74 22:21:24.02 +42:26:35.3
95.55065 -12.31325 galactic Lac Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1958542199793256960 | 22:21:24.01 +42:26:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.262+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:24.02 +42:26:35.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:24.02 +42:26:35.3: 12.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 1958542199793256960,2461177.9465,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958542199793256960 20260517.4465 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.80 22:12:22.03 +33:37:10.1
88.75955 -18.49326 galactic Peg Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1899339889547890816 | 22:12:22.04 +33:37:11.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.385+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:22.03 +33:37:10.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:22.03 +33:37:10.1: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1899339889547890816,2461177.9465,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899339889547890816 20260517.4465 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.95 22:21:42.00 +36:19:17.1
92.04924 -17.41572 galactic Lac Second-epoch detections are separated by 0.3" and 7.3 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 1906006469065113728 | 22:21:42.10 +36:19:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:42.00 +36:19:17.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:42.00 +36:19:17.1: 12.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 1906006469065113728,2461177.9465,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1906006469065113728 20260517.4465 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.93 22:17:48.84 +33:39:27.3
89.74796 -19.13461 galactic Peg Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905121843240986624 | 22:17:48.88 +33:39:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:48.84 +33:39:27.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:48.84 +33:39:27.3: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1905121843240986624,2461177.9465,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905121843240986624 20260517.4465 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.95 22:19:37.01 +33:46:32.0
90.14339 -19.25711 galactic Peg Second-epoch detections are separated by 0.1" and 7.5 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 J334.9083+33.7876 | 22:19:37.01 +33:46:32.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.270+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:37.01 +33:46:32.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:37.01 +33:46:32.0: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 J334.9083+33.7876,2461177.9465,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.9083+33.7876 20260517.4465 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.96 22:26:48.54 +40:52:45.2
95.53803 -14.17495 galactic Lac Second-epoch detections are separated by 0.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1909383172354020096 | 22:26:48.57 +40:52:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.144+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:48.54 +40:52:45.2: 13.07 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:48.54 +40:52:45.2: 12.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 1909383172354020096,2461177.9465,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1909383172354020096 20260517.4465 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 9.61 22:23:00.39 +33:22:31.9
90.51188 -19.99062 galactic Peg Second-epoch detections are separated by 0.8" and 7.4 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 1902144327094668416 | 22:23:00.34 +33:22:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:00.39 +33:22:31.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:00.39 +33:22:31.9: 12.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 1902144327094668416,2461177.9465,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902144327094668416 20260517.4465 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.14 22:27:11.63 +39:57:46.0
95.08844 -14.98483 galactic Lac Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1909272911953160320 | 22:27:11.64 +39:57:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.325+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:11.63 +39:57:46.0: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:11.63 +39:57:46.0: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 1909272911953160320,2461177.9465,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1909272911953160320 20260517.4465 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.31 22:28:34.78 +39:09:23.3
94.86886 -15.80742 galactic Lac Second-epoch detections are separated by 2.0" and 7.3 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 J337.1411+39.1471 | 22:28:34.85 +39:09:25.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.656+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:34.78 +39:09:23.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:34.78 +39:09:23.3: 13.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J337.1411+39.1471,2461177.9465,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J337.1411+39.1471 20260517.4465 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.04 22:29:17.70 +41:28:01.8
96.27040 -13.93042 galactic Lac Second-epoch detections are separated by 1.2" and 7.0 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 J337.3237+41.4676 | 22:29:17.70 +41:28:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:17.70 +41:28:01.8: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:17.70 +41:28:01.8: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 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
ATO J337.3237+41.4676,2461177.9465,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J337.3237+41.4676 20260517.4465 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.26 22:25:28.17 +39:24:20.4
94.48560 -15.27078 galactic Lac Second-epoch detections are separated by 0.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1908877736303214208 | 22:25:28.24 +39:24:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:28.17 +39:24:20.4: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:28.17 +39:24:20.4: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 1908877736303214208,2461177.9465,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1908877736303214208 20260517.4465 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.32 22:25:38.23 +42:04:06.0
96.01162 -13.05677 galactic Lac Second-epoch detections are separated by 0.5" and 6.7 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 | 22:25:38.23 +42:04:06.0 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:38.23 +42:04:06.0: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:38.23 +42:04:06.0: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 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
target,2461177.9465,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.29 22:27:53.47 +39:12:46.6
94.78401 -15.68776 galactic Lac Second-epoch detections are separated by 0.2" and 7.0 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 | 22:27:53.47 +39:12:46.6 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:53.47 +39:12:46.6: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:53.47 +39:12:46.6: 13.29 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.33 22:18:03.70 +34:22:51.4
90.23827 -18.57731 galactic Peg Second-epoch detections are separated by 1.1" and 7.5 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 | 22:18:03.70 +34:22:51.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.286+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:03.70 +34:22:51.4: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:03.70 +34:22:51.4: 13.49 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.10 22:21:12.83 +33:36:39.6
90.33005 -19.58336 galactic Peg Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.3032+33.6129 | 22:21:12.83 +33:36:39.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:12.83 +33:36:39.6: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:12.83 +33:36:39.6: 13.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.24 +/- 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
ATO J335.3032+33.6129,2461177.9465,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.3032+33.6129 20260517.4465 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.62 22:24:01.72 +41:06:40.3
95.21538 -13.69435 galactic Lac Second-epoch detections are separated by 0.8" and 6.8 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 | 22:24:01.72 +41:06:40.3 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:01.72 +41:06:40.3: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:01.72 +41:06:40.3: 13.50 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.29 22:26:23.97 +39:12:20.6
94.52821 -15.53659 galactic Lac Second-epoch detections are separated by 0.2" and 7.1 pix
The object was found in VSX 2" Gaia DR3 1908672750402617600
Type: VAR
# Max. Min./Amp. JD0 Period
12.570 G 17.530 G 0.041685100000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:23.97 +39:12:20.6: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:23.97 +39:12:20.6: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 1908672750402617600,2461177.9465,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1908672750402617600 20260517.4465 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.65 22:21:24.82 +42:13:35.3
95.42966 -12.49487 galactic Lac Second-epoch detections are separated by 1.2" and 6.6 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 | 22:21:24.82 +42:13:35.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:24.82 +42:13:35.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:24.82 +42:13:35.3: 13.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.51 22:24:41.50 +41:00:03.8
95.26078 -13.85500 galactic Lac Second-epoch detections are separated by 0.5" and 6.9 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 J336.1583+41.0030 | 22:24:41.50 +41:00:03.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:41.50 +41:00:03.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:41.50 +41:00:03.8: 13.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J336.1583+41.0030,2461177.9465,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J336.1583+41.0030 20260517.4465 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 05 17.4465 2461177.9465 10.44 22:26:22.34 +40:13:20.2
95.09783 -14.68161 galactic Lac Second-epoch detections are separated by 0.4" and 6.9 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 | 22:26:22.34 +40:13:20.2 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.031 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:22.34 +40:13:20.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:22.34 +40:13:20.2: 13.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.35 +/- 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
target,2461177.9465,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.49 22:24:21.93 +37:53:05.3
93.42606 -16.41995 galactic Lac Second-epoch detections are separated by 0.6" and 7.2 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 | 22:24:21.93 +37:53:05.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:21.93 +37:53:05.3: 12.27 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:21.93 +37:53:05.3: 13.60 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.23 +/- 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
target,2461177.9465,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.68 22:20:34.64 +41:55:56.8
95.12991 -12.65280 galactic Lac Second-epoch detections are separated by 0.8" and 6.7 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 J335.1491+41.9350 | 22:20:34.64 +41:55:56.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.335+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:34.64 +41:55:56.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:34.64 +41:55:56.8: 13.53 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.1491+41.9350,2461177.9465,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.1491+41.9350 20260517.4465 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.55 22:28:36.85 +41:59:19.6
96.44620 -13.42146 galactic Lac Second-epoch detections are separated by 0.6" and 6.8 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 | 22:28:36.85 +41:59:19.6 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:36.85 +41:59:19.6: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:36.85 +41:59:19.6: 13.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.71 22:29:26.98 +40:50:01.7
95.94735 -14.48171 galactic Lac Second-epoch detections are separated by 0.6" and 6.9 pix
The object was found in VSX 2" Gaia DR3 1909417806969836544
Type: ROT
# Max. Min./Amp. JD0 Period
12.780 G 12.800 G 24.604000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:26.98 +40:50:01.7: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:26.98 +40:50:01.7: 13.60 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1909417806969836544,2461177.9465,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1909417806969836544 20260517.4465 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.42 22:01:47.47 +34:07:04.1
87.26172 -16.75258 galactic Peg Second-epoch detections are separated by 0.3" and 7.5 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 | 22:01:47.47 +34:07:04.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:47.47 +34:07:04.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:47.47 +34:07:04.1: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 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,2461177.9465,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 17.4465 2461177.9465 10.78 22:29:25.90 +39:41:13.8
95.30939 -15.44864 galactic Lac Second-epoch detections are separated by 3.3" and 7.3 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 | 22:29:25.90 +39:41:13.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:25.90 +39:41:13.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:25.90 +39:41:13.8: 13.87 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461177.9465,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260517.4465 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461177.94681082 17.05.2026 10:43:14.455 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23503
Objects passed selection criteria: 23491
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 22815.5
Average stars matched: 22452.2 (98.4079 %)
Memory usage VmPeak: 127868 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 17 08:03:36 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461177.94681082 17.05.2026 10:43:14.455 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 202
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 111 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): 132721
Objects passed selection criteria: 132522
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 134197
Average stars matched: 132174 (98.4925 %)
Memory usage VmPeak: 1979624 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 17 08:07:58 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
SExtractor catalog cache: saved Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461177.94627731
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits exists and is non-empty
Saving wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits to local_wcs_cache/
'wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits'
wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (1st reference image)
verification OK: wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Image size: 932.3'x637.3' 15.5(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.99"/pix along the Y axis
Image center: 21:48:57.820 +38:02:09.57 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 21:49:04.910 +38:00:05.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:04.910 +38:00:05.47
Angular distance between the image centers 0.0416 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 21:49:07.661 +37:59:35.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:07.661 +37:59:35.70
Angular distance between the image centers 0.0536 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:49:04.910 +38:00:05.47
Second-epoch second image center 21:49:07.661 +37:59:35.70
Angular distance between the image centers 0.01225 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.WijRczBWYk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits &> /tmp/tmp.0evc8IIKmr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits &> /tmp/tmp.yGplnPKi0r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits &> /tmp/tmp.p3bItIcdUR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Found non-empty wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
The reference image (wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits) and catalog (wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat) found
'wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.968900
a=0.000000 b=1.000000 c=22.968900
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (aperture=6.2)
Read 21746 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5217 to 337.7622 deg, Dec +32.2988 to +43.2789 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.5217 to 337.7622 deg, Dec 32.2988 to 43.2789 deg
Loaded 21125 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 13298 out of 14228 total matches.
Matched with Tycho-2 14228 out of 21746 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -> calib.txt_param_ref_wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits (aperture=7.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
4.0 pix fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
4.0 pix fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
2.2 pix wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Limiting magnitude estimates:
15.2 mag. Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
14.7 mag. Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
14.5 mag. fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
14.5 mag. fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.WijRczBWYk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2960, passed=28429
Got 28429 stars (including 25433 good ones) from the SExtractor catalog wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 28429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 424 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 377 matched stars entering correct_measured_positions(), 326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 373 matched stars entering correct_measured_positions(), 11634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 495 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 453 matched stars entering correct_measured_positions(), 11686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
Accuracy estimation diagnostic: 452 matched stars entering correct_measured_positions(), 13987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
Excluding outliers - 452 stars left (next iteration limit 410)
WCS_QUALITY_DIAG: file=Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits N_match=452 sigma_overall_arcsec=5.245 sigma_q1_arcsec=26.359 sigma_q2_arcsec=5.045 sigma_q3_arcsec=33.611 sigma_q4_arcsec=3.580 n_q1=17 n_q2=196 n_q3=13 n_q4=226 worst_quadrant_to_overall_ratio=6.408
The image catalog is written to wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0evc8IIKmr (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS-calibrated image found: wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Checking if the catalog wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS catalog name: wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1940, passed=21746
Got 21746 stars (including 19798 good ones) from the SExtractor catalog wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
util/solve_plate_with_UCAC5 got 21746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits N_match=958 sigma_overall_arcsec=0.835 sigma_q1_arcsec=0.743 sigma_q2_arcsec=0.865 sigma_q3_arcsec=0.787 sigma_q4_arcsec=1.356 n_q1=279 n_q2=167 n_q3=304 n_q4=208 worst_quadrant_to_overall_ratio=1.624
The image catalog is written to wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -region wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yGplnPKi0r (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
Checking if the catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
WCS catalog name: wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1165, passed=21136
Got 21136 stars (including 19963 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat
util/solve_plate_with_UCAC5 got 21136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 20813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 20816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 20816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits N_match=951 sigma_overall_arcsec=0.454 sigma_q1_arcsec=0.569 sigma_q2_arcsec=0.517 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.421 n_q1=246 n_q2=183 n_q3=313 n_q4=209 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits -region wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.p3bItIcdUR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
Checking if the catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
WCS catalog name: wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1148, passed=20516
Got 20516 stars (including 19357 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat
util/solve_plate_with_UCAC5 got 20516 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 20216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 20215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 20215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits N_match=951 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.521 sigma_q2_arcsec=0.541 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.457 n_q1=244 n_q2=183 n_q3=315 n_q4=209 worst_quadrant_to_overall_ratio=1.233
The image catalog is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits -region wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits sigma_overall=5.245 worst_q_ratio=6.408
ref2=Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits sigma_overall=0.835 worst_q_ratio=1.624
new1=fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits sigma_overall=0.454 worst_q_ratio=1.253
new2=fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits sigma_overall=0.438 worst_q_ratio=1.233
reference average sigma_overall=3.04 worst_q_ratio=4.016
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041_astrometric_residuals.png (452 matched stars from wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728_astrometric_residuals.png (958 matched stars from wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484_astrometric_residuals.png (951 matched stars from wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485_astrometric_residuals.png (951 matched stars from wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-42-28_20.00sec_-0.00C_LIGHTs_0484.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Cyg-07-Q1b1x1_054807_TTUQ1b1x1_4122012_dAtLIlTf/wcs_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485.fits'
Preparing the HTML report for the field Cyg-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:51.22 +39:18:54.4: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:22.19 +38:18:45.8: 15.14 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:06.83 +39:56:16.5: 14.92 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:47.42 +37:36:36.1: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:49.49 +40:42:50.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:22.25 +42:20:25.3: 13.96 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:22.19 +38:18:45.8: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:49.49 +40:42:50.2: 12.05 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:32.93 +41:39:12.1: 15.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.05 +/- 0.02
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry filter REJECTED candidate at 21:36:49.49 +40:42:50.2: ref_mag=12.05 +/- 0.02 new_mean_mag=12.1297 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:49:22.19 +38:18:45.8: ref_mag=12.30 +/- 0.02 new_mean_mag=12.0208 delta=0.28 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:47.42 +37:36:36.1: 12.16 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:06.83 +39:56:16.5: 12.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry filter REJECTED candidate at 21:56:47.42 +37:36:36.1: ref_mag=12.16 +/- 0.02 new_mean_mag=12.0467 delta=0.11 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:30:10.79 +40:59:20.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:48.56 +41:19:49.6: 14.25 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Forced photometry filter REJECTED candidate at 21:28:06.83 +39:56:16.5: ref_mag=12.79 +/- 0.03 new_mean_mag=12.0216 delta=0.77 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:51.22 +39:18:54.4: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Forced photometry filter REJECTED candidate at 22:01:51.22 +39:18:54.4: ref_mag=10.63 +/- 0.00 new_mean_mag=10.9501 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:09.23 +42:44:06.7: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:22.25 +42:20:25.3: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.02
Forced photometry filter REJECTED candidate at 21:33:22.25 +42:20:25.3: ref_mag=12.12 +/- 0.02 new_mean_mag=12.0993 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:32.93 +41:39:12.1: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.03
Forced photometry filter REJECTED candidate at 22:22:32.93 +41:39:12.1: ref_mag=12.54 +/- 0.03 new_mean_mag=12.2541 delta=0.29 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:30:10.79 +40:59:20.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:30:10.79 +40:59:20.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:48.56 +41:19:49.6: 11.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.02
Forced photometry filter REJECTED candidate at 21:09:48.56 +41:19:49.6: ref_mag=11.95 +/- 0.02 new_mean_mag=12.2695 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:09.23 +42:44:06.7: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.02
Forced photometry filter REJECTED candidate at 21:21:09.23 +42:44:06.7: ref_mag=12.08 +/- 0.02 new_mean_mag=12.1861 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:18.03 +39:19:42.8: 13.55 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:18.03 +39:19:42.8: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.03
Forced photometry filter REJECTED candidate at 21:17:18.03 +39:19:42.8: ref_mag=12.48 +/- 0.03 new_mean_mag=12.3222 delta=0.16 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31037_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31037_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31150_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31150_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 22:25:45.67 +38:49:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31215_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31215_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:14:57.18 +38:02:08.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31250_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31250_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:21:01.08 +40:03:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31265_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31265_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:15:54.81 +38:11:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31289_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31289_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31307_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31307_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31310_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31310_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31312_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31312_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31314_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31314_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31325_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31325_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31359_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31359_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31362_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31362_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31365_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31365_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 31366_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31366_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 22:10:34.38 +40:35:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31370_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 31370_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 30014_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 30014_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 22:10:36.40 +41:28:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218204_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218204_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218206_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218206_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218208_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218208_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218214_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218214_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218215_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218215_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218230_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218230_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218235_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218235_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218242_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218242_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218248_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218248_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218250_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218250_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218254_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218254_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218257_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218257_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218258_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218258_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218260_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218260_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218261_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218261_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218262_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218262_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218322_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218322_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218476_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218476_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218481_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218481_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218525_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218525_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218548_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218548_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 22:23:22.07 +42:04:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218593_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218593_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218646_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218646_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:17:35.80 +39:23:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218675_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218675_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:19:04.86 +39:43:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218761_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218761_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:09:40.85 +42:24:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218783_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218783_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:19:02.00 +41:01:25.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218821_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218821_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218839_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218839_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218863_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218863_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:12:19.71 +40:08:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218866_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218866_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218893_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218893_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218908_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218908_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:13:19.06 +35:28:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218909_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218909_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:13:23.97 +40:26:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218925_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218925_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218930_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218930_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:09:45.84 +41:39:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218939_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218939_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:49:11.22 +42:20:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218961_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218961_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:14:53.20 +38:04:33.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 218962_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218962_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218963_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218963_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 218991_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 218991_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 218993_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 218993_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:55:32.69 +43:01:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219014_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219014_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:49:16.03 +43:03:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219021_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219021_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219044_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219044_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:11:53.33 +36:50:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219045_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219045_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219047_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219047_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:11:02.15 +38:21:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219093_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219093_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219104_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219104_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219108_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219108_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 22:25:55.52 +41:56:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219114_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219114_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:14:27.25 +38:46:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219116_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219116_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:31:08.87 +43:06:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219118_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219118_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219127_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219127_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219160_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219160_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:19:57.20 +43:06:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219174_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219174_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219198_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219198_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219199_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219199_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219211_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219211_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219229_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219229_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219230_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219230_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219233_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219233_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219236_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219236_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:31:19.13 +41:47:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219251_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219251_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219272_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219272_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219273_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219273_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219302_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219302_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219305_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219305_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:09:38.34 +40:37:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219313_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219313_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219318_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219318_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:21:14.29 +41:13:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219319_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219319_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:09:41.82 +40:35:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219321_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219321_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:21:30.17 +41:54:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219331_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219331_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219340_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219340_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219346_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219346_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219354_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219354_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219358_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219358_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219419_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219419_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219434_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219434_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219437_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219437_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219440_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219440_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219477_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219477_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
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Considering the candidate 219482_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219482_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:20:24.72 +37:37:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219483_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219483_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:34:52.31 +41:17:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219504_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219504_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219505_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219505_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219518_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219518_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219519_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219519_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219520_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219520_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219546_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219546_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 22:13:05.09 +41:48:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219547_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219547_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219561_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219561_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:15:01.90 +41:23:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219566_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219566_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:55:27.23 +42:00:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219586_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219586_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219595_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219595_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:55:01.49 +42:15:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219645_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219645_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219658_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 219658_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 219691_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219691_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219693_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219693_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219712_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219712_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219766_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219766_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219786_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219786_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219789_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219789_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 219792_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 219792_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 13745_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 13745_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212246_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212246_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 213138_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 213138_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 65438_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 65438_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 33331_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 33331_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:26:52.23 +41:39:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215029_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 215029_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:11:35.52 +40:34:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67601_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 67601_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 172732_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 172732_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 213234_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 213234_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 42459_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 42459_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:18:30.89 +41:07:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213049_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 213049_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212973_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212973_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212860_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212860_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212849_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212849_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212847_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212847_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212795_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212795_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212696_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212696_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212591_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212591_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212544_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212544_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212539_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212539_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212538_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212538_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 102295_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 102295_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:15:54.95 +38:11:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212497_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212497_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212454_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212454_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212438_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212438_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212431_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212431_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212411_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212411_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212363_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212363_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212353_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212353_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212321_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212321_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212312_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212312_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212306_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212306_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212263_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212263_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 212199_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 212199_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 174323_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 174323_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
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Considering the candidate 03628_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
The candidate 03628_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485 did not pass the final checks
**** FOUND 21:19:49.17 +43:04:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57529_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
Preparing report for the candidate 57529_fd_Cyg-07-Q1b1x1_2026-05-17_05-43-14_20.00sec_-0.00C_LIGHTs_0485
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 222s
Prepared the HTML report for the field Cyg-07-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:28:16.88 +41:56:37.5
21:13:42.11 +34:07:20.2
22:01:47.47 +34:07:04.1
22:29:26.98 +40:50:01.7
22:24:47.79 +41:23:33.9
22:28:36.85 +41:59:19.6
22:20:34.64 +41:55:56.8
22:24:21.93 +37:53:05.3
22:26:22.34 +40:13:20.2
22:24:41.50 +41:00:03.8
22:21:24.82 +42:13:35.3
22:26:23.97 +39:12:20.6
22:24:01.72 +41:06:40.3
22:21:12.83 +33:36:39.6
22:18:03.70 +34:22:51.4
22:27:53.47 +39:12:46.6
22:25:38.23 +42:04:06.0
22:25:28.17 +39:24:20.4
22:29:17.70 +41:28:01.8
22:28:34.78 +39:09:23.3
22:27:11.63 +39:57:46.0
22:23:00.39 +33:22:31.9
22:26:48.54 +40:52:45.2
22:19:37.01 +33:46:32.0
22:17:48.84 +33:39:27.3
22:21:42.00 +36:19:17.1
22:12:22.03 +33:37:10.1
22:25:18.24 +34:10:33.3
22:21:24.02 +42:26:35.3
21:31:28.72 +39:48:09.6
22:23:52.17 +39:48:15.6
22:17:40.49 +40:49:15.2
21:16:59.17 +37:32:52.5
22:22:14.11 +41:40:45.7
21:54:37.12 +36:25:58.5
21:12:16.07 +34:09:55.3
22:01:22.35 +40:55:07.5
21:21:02.46 +42:07:14.1
22:24:29.08 +33:18:07.3
21:47:22.88 +33:57:51.4
21:57:39.28 +41:47:18.1
21:14:24.68 +33:06:52.2
22:20:17.38 +34:47:25.5
21:11:40.23 +34:59:54.3
21:48:47.02 +40:08:13.0
21:12:49.69 +41:23:26.1
21:33:38.23 +37:37:16.6
21:33:10.78 +39:46:10.6
22:27:29.73 +41:09:13.6
21:28:08.25 +36:39:03.2
21:20:25.20 +37:31:57.8
22:05:08.02 +36:40:55.1
22:01:07.90 +39:15:18.8
21:31:14.85 +38:46:29.2
22:29:53.29 +41:25:59.8
21:15:49.53 +38:27:47.2
21:21:47.75 +35:29:49.3
21:17:37.36 +36:35:15.1
22:20:55.87 +41:36:25.0
21:26:25.15 +35:51:23.8
21:17:44.37 +33:45:12.6
22:02:13.83 +41:47:07.6
22:07:05.43 +37:55:15.5
22:26:44.90 +40:34:43.6
21:24:39.60 +36:58:44.7
22:07:49.41 +33:25:38.1
21:58:07.66 +38:56:39.7
21:35:16.75 +37:59:46.9
21:17:23.18 +41:27:44.6
21:29:07.94 +42:01:02.3
21:57:40.54 +37:18:47.0
21:15:42.90 +33:53:34.2
21:20:52.04 +38:17:39.3
21:48:37.93 +41:48:10.0
21:18:35.07 +40:16:41.5
21:16:29.73 +36:57:21.7
21:14:44.85 +38:12:02.9
22:06:31.85 +34:33:34.9
21:34:48.95 +41:16:17.1
22:17:36.78 +42:32:37.0
22:06:46.45 +39:39:12.0
21:42:06.01 +36:50:53.5
22:20:30.92 +33:33:33.5
21:10:36.26 +40:19:47.7
22:26:17.79 +40:38:19.1
22:15:17.67 +39:47:52.8
22:03:59.71 +39:46:37.0
21:29:05.00 +40:27:03.4
22:14:09.55 +38:28:25.4
21:25:05.40 +37:46:26.3
21:27:59.53 +37:32:20.0
21:44:49.60 +36:56:52.9
21:42:23.21 +40:36:52.9
22:04:58.72 +32:49:10.1
22:01:13.37 +38:32:59.7
21:14:48.61 +37:08:04.4
21:43:31.98 +38:44:13.9
22:21:21.30 +41:17:35.5
22:09:11.47 +36:46:04.4
21:24:42.34 +38:26:37.6
21:27:07.29 +35:14:56.3
22:02:04.62 +37:45:26.7
22:29:25.90 +39:41:13.8
22:25:05.70 +39:23:43.0
21:28:06.80 +39:56:16.2
########### Completed Cyg-07-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:31:28.72 +39:48:09.6
22:23:52.17 +39:48:15.6
22:17:40.49 +40:49:15.2
21:16:59.17 +37:32:52.5
22:22:14.11 +41:40:45.7
21:54:37.12 +36:25:58.5
21:12:16.07 +34:09:55.3
22:01:22.35 +40:55:07.5
21:21:02.46 +42:07:14.1
22:24:29.08 +33:18:07.3
21:47:22.88 +33:57:51.4
21:57:39.28 +41:47:18.1
21:14:24.68 +33:06:52.2
22:20:17.38 +34:47:25.5
21:11:40.23 +34:59:54.3
21:48:47.02 +40:08:13.0
21:12:49.69 +41:23:26.1
21:33:38.23 +37:37:16.6
21:33:10.78 +39:46:10.6
22:27:29.73 +41:09:13.6
21:28:08.25 +36:39:03.2
21:20:25.20 +37:31:57.8
22:05:08.02 +36:40:55.1
22:01:07.90 +39:15:18.8
21:31:14.85 +38:46:29.2
22:29:53.29 +41:25:59.8
21:15:49.53 +38:27:47.2
21:21:47.75 +35:29:49.3
21:17:37.36 +36:35:15.1
22:20:55.87 +41:36:25.0
21:26:25.15 +35:51:23.8
21:17:44.37 +33:45:12.6
22:02:13.83 +41:47:07.6
22:07:05.43 +37:55:15.5
22:26:44.90 +40:34:43.6
21:24:39.60 +36:58:44.7
22:07:49.41 +33:25:38.1
21:58:07.66 +38:56:39.7
21:35:16.75 +37:59:46.9
21:17:23.18 +41:27:44.6
21:29:07.94 +42:01:02.3
21:57:40.54 +37:18:47.0
21:15:42.90 +33:53:34.2
21:20:52.04 +38:17:39.3
21:48:37.93 +41:48:10.0
21:18:35.07 +40:16:41.5
21:16:29.73 +36:57:21.7
21:14:44.85 +38:12:02.9
22:06:31.85 +34:33:34.9
21:34:48.95 +41:16:17.1
22:17:36.78 +42:32:37.0
22:06:46.45 +39:39:12.0
21:42:06.01 +36:50:53.5
22:20:30.92 +33:33:33.5
21:10:36.26 +40:19:47.7
22:26:17.79 +40:38:19.1
22:15:17.67 +39:47:52.8
22:03:59.71 +39:46:37.0
21:29:05.00 +40:27:03.4
22:14:09.55 +38:28:25.4
21:25:05.40 +37:46:26.3
21:27:59.53 +37:32:20.0
21:44:49.60 +36:56:52.9
21:42:23.21 +40:36:52.9
22:04:58.72 +32:49:10.1
22:01:13.37 +38:32:59.7
21:14:48.61 +37:08:04.4
21:43:31.98 +38:44:13.9
22:21:21.30 +41:17:35.5
22:09:11.47 +36:46:04.4
21:24:42.34 +38:26:37.6
21:27:07.29 +35:14:56.3
22:02:04.62 +37:45:26.7
22:28:16.88 +41:56:37.5
22:24:47.79 +41:23:33.9
22:25:18.24 +34:10:33.3
22:25:05.70 +39:23:43.0
21:28:06.80 +39:56:16.2
21:13:42.11 +34:07:20.2
22:21:24.02 +42:26:35.3
22:12:22.03 +33:37:10.1
22:21:42.00 +36:19:17.1
22:17:48.84 +33:39:27.3
22:19:37.01 +33:46:32.0
22:26:48.54 +40:52:45.2
22:23:00.39 +33:22:31.9
22:27:11.63 +39:57:46.0
22:28:34.78 +39:09:23.3
22:29:17.70 +41:28:01.8
22:25:28.17 +39:24:20.4
22:25:38.23 +42:04:06.0
22:27:53.47 +39:12:46.6
22:18:03.70 +34:22:51.4
22:21:12.83 +33:36:39.6
22:24:01.72 +41:06:40.3
22:26:23.97 +39:12:20.6
22:21:24.82 +42:13:35.3
22:24:41.50 +41:00:03.8
22:26:22.34 +40:13:20.2
22:24:21.93 +37:53:05.3
22:20:34.64 +41:55:56.8
22:28:36.85 +41:59:19.6
22:29:26.98 +40:50:01.7
22:01:47.47 +34:07:04.1
22:29:25.90 +39:41:13.8
###################################################################################
21:31:28.72 +39:48:09.6 -- not an asteroid (will add it to exclusion list)
22:23:52.17 +39:48:15.6 -- not an asteroid (will add it to exclusion list)
22:17:40.49 +40:49:15.2 -- not an asteroid (will add it to exclusion list)
21:16:59.17 +37:32:52.5 -- not an asteroid (will add it to exclusion list)
22:22:14.11 +41:40:45.7 -- not an asteroid (will add it to exclusion list)
21:54:37.12 +36:25:58.5 -- not an asteroid (will add it to exclusion list)
21:12:16.07 +34:09:55.3 -- not an asteroid (will add it to exclusion list)
22:01:22.35 +40:55:07.5 -- not an asteroid (will add it to exclusion list)
21:21:02.46 +42:07:14.1 -- not an asteroid (will add it to exclusion list)
22:24:29.08 +33:18:07.3 -- not an asteroid (will add it to exclusion list)
21:47:22.88 +33:57:51.4 -- not an asteroid (will add it to exclusion list)
21:57:39.28 +41:47:18.1 -- not an asteroid (will add it to exclusion list)
21:14:24.68 +33:06:52.2 -- not an asteroid (will add it to exclusion list)
22:20:17.38 +34:47:25.5 -- not an asteroid (will add it to exclusion list)
21:11:40.23 +34:59:54.3 -- not an asteroid (will add it to exclusion list)
21:48:47.02 +40:08:13.0 -- not an asteroid (will add it to exclusion list)
21:12:49.69 +41:23:26.1 -- not an asteroid (will add it to exclusion list)
21:33:38.23 +37:37:16.6 -- not an asteroid (will add it to exclusion list)
21:33:10.78 +39:46:10.6 -- not an asteroid (will add it to exclusion list)
22:27:29.73 +41:09:13.6 -- not an asteroid (will add it to exclusion list)
21:28:08.25 +36:39:03.2 -- not an asteroid (will add it to exclusion list)
21:20:25.20 +37:31:57.8 -- not an asteroid (will add it to exclusion list)
22:05:08.02 +36:40:55.1 -- not an asteroid (will add it to exclusion list)
22:01:07.90 +39:15:18.8 -- not an asteroid (will add it to exclusion list)
21:31:14.85 +38:46:29.2 -- not an asteroid (will add it to exclusion list)
22:29:53.29 +41:25:59.8 -- not an asteroid (will add it to exclusion list)
21:15:49.53 +38:27:47.2 -- not an asteroid (will add it to exclusion list)
21:21:47.75 +35:29:49.3 -- not an asteroid (will add it to exclusion list)
21:17:37.36 +36:35:15.1 -- not an asteroid (will add it to exclusion list)
22:20:55.87 +41:36:25.0 -- not an asteroid (will add it to exclusion list)
21:26:25.15 +35:51:23.8 -- not an asteroid (will add it to exclusion list)
21:17:44.37 +33:45:12.6 -- not an asteroid (will add it to exclusion list)
22:02:13.83 +41:47:07.6 -- not an asteroid (will add it to exclusion list)
22:07:05.43 +37:55:15.5 -- not an asteroid (will add it to exclusion list)
22:26:44.90 +40:34:43.6 -- not an asteroid (will add it to exclusion list)
21:24:39.60 +36:58:44.7 -- not an asteroid (will add it to exclusion list)
22:07:49.41 +33:25:38.1 -- not an asteroid (will add it to exclusion list)
21:58:07.66 +38:56:39.7 -- not an asteroid (will add it to exclusion list)
21:35:16.75 +37:59:46.9 -- not an asteroid (will add it to exclusion list)
21:17:23.18 +41:27:44.6 -- not an asteroid (will add it to exclusion list)
21:29:07.94 +42:01:02.3 -- not an asteroid (will add it to exclusion list)
21:57:40.54 +37:18:47.0 -- not an asteroid (will add it to exclusion list)
21:15:42.90 +33:53:34.2 -- not an asteroid (will add it to exclusion list)
21:20:52.04 +38:17:39.3 -- not an asteroid (will add it to exclusion list)
21:48:37.93 +41:48:10.0 -- not an asteroid (will add it to exclusion list)
21:18:35.07 +40:16:41.5 -- not an asteroid (will add it to exclusion list)
21:16:29.73 +36:57:21.7 -- not an asteroid (will add it to exclusion list)
21:14:44.85 +38:12:02.9 -- not an asteroid (will add it to exclusion list)
22:06:31.85 +34:33:34.9 -- not an asteroid (will add it to exclusion list)
21:34:48.95 +41:16:17.1 -- not an asteroid (will add it to exclusion list)
22:17:36.78 +42:32:37.0 -- not an asteroid (will add it to exclusion list)
22:06:46.45 +39:39:12.0 -- not an asteroid (will add it to exclusion list)
21:42:06.01 +36:50:53.5 -- not an asteroid (will add it to exclusion list)
22:20:30.92 +33:33:33.5 -- not an asteroid (will add it to exclusion list)
21:10:36.26 +40:19:47.7 -- not an asteroid (will add it to exclusion list)
22:26:17.79 +40:38:19.1 -- not an asteroid (will add it to exclusion list)
22:15:17.67 +39:47:52.8 -- not an asteroid (will add it to exclusion list)
22:03:59.71 +39:46:37.0 -- not an asteroid (will add it to exclusion list)
21:29:05.00 +40:27:03.4 -- not an asteroid (will add it to exclusion list)
22:14:09.55 +38:28:25.4 -- not an asteroid (will add it to exclusion list)
21:25:05.40 +37:46:26.3 -- not an asteroid (will add it to exclusion list)
21:27:59.53 +37:32:20.0 -- not an asteroid (will add it to exclusion list)
21:44:49.60 +36:56:52.9 -- not an asteroid (will add it to exclusion list)
21:42:23.21 +40:36:52.9 -- not an asteroid (will add it to exclusion list)
22:04:58.72 +32:49:10.1 -- not an asteroid (will add it to exclusion list)
22:01:13.37 +38:32:59.7 -- not an asteroid (will add it to exclusion list)
21:14:48.61 +37:08:04.4 -- not an asteroid (will add it to exclusion list)
21:43:31.98 +38:44:13.9 -- not an asteroid (will add it to exclusion list)
22:21:21.30 +41:17:35.5 -- not an asteroid (will add it to exclusion list)
22:09:11.47 +36:46:04.4 -- not an asteroid (will add it to exclusion list)
21:24:42.34 +38:26:37.6 -- not an asteroid (will add it to exclusion list)
21:27:07.29 +35:14:56.3 -- not an asteroid (will add it to exclusion list)
22:02:04.62 +37:45:26.7 -- not an asteroid (will add it to exclusion list)
22:28:16.88 +41:56:37.5 -- not an asteroid (will add it to exclusion list)
22:24:47.79 +41:23:33.9 -- not an asteroid (will add it to exclusion list)
22:25:18.24 +34:10:33.3 -- not an asteroid (will add it to exclusion list)
22:25:05.70 +39:23:43.0 -- not an asteroid (will add it to exclusion list)
21:28:06.80 +39:56:16.2 -- not an asteroid (will add it to exclusion list)
21:13:42.11 +34:07:20.2 -- not an asteroid (will add it to exclusion list)
22:21:24.02 +42:26:35.3 -- not an asteroid (will add it to exclusion list)
22:12:22.03 +33:37:10.1 -- not an asteroid (will add it to exclusion list)
22:21:42.00 +36:19:17.1 -- not an asteroid (will add it to exclusion list)
22:17:48.84 +33:39:27.3 -- not an asteroid (will add it to exclusion list)
22:19:37.01 +33:46:32.0 -- not an asteroid (will add it to exclusion list)
22:26:48.54 +40:52:45.2 -- not an asteroid (will add it to exclusion list)
22:23:00.39 +33:22:31.9 -- not an asteroid (will add it to exclusion list)
22:27:11.63 +39:57:46.0 -- not an asteroid (will add it to exclusion list)
22:28:34.78 +39:09:23.3 -- not an asteroid (will add it to exclusion list)
22:29:17.70 +41:28:01.8 -- not an asteroid (will add it to exclusion list)
22:25:28.17 +39:24:20.4 -- not an asteroid (will add it to exclusion list)
22:25:38.23 +42:04:06.0 -- not an asteroid (will add it to exclusion list)
22:27:53.47 +39:12:46.6 -- not an asteroid (will add it to exclusion list)
22:18:03.70 +34:22:51.4 -- not an asteroid (will add it to exclusion list)
22:21:12.83 +33:36:39.6 -- not an asteroid (will add it to exclusion list)
22:24:01.72 +41:06:40.3 -- not an asteroid (will add it to exclusion list)
22:26:23.97 +39:12:20.6 -- not an asteroid (will add it to exclusion list)
22:21:24.82 +42:13:35.3 -- not an asteroid (will add it to exclusion list)
22:24:41.50 +41:00:03.8 -- not an asteroid (will add it to exclusion list)
22:26:22.34 +40:13:20.2 -- not an asteroid (will add it to exclusion list)
22:24:21.93 +37:53:05.3 -- not an asteroid (will add it to exclusion list)
22:20:34.64 +41:55:56.8 -- not an asteroid (will add it to exclusion list)
22:28:36.85 +41:59:19.6 -- not an asteroid (will add it to exclusion list)
22:29:26.98 +40:50:01.7 -- not an asteroid (will add it to exclusion list)
22:01:47.47 +34:07:04.1 -- not an asteroid (will add it to exclusion list)
22:29:25.90 +39:41:13.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:10:36.26 +40:19:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:40.23 +34:59:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:16.07 +34:09:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:49.69 +41:23:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:42.11 +34:07:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:24.68 +33:06:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:44.85 +38:12:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:48.61 +37:08:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:42.90 +33:53:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:49.53 +38:27:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:29.73 +36:57:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:59.17 +37:32:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:23.18 +41:27:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:37.36 +36:35:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:44.37 +33:45:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:35.07 +40:16:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:25.20 +37:31:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:52.04 +38:17:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:02.46 +42:07:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:47.75 +35:29:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:39.60 +36:58:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:42.34 +38:26:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:05.40 +37:46:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:25.15 +35:51:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:07.29 +35:14:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:59.53 +37:32:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.80 +39:56:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:08.25 +36:39:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:05.00 +40:27:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:07.94 +42:01:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.85 +38:46:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.72 +39:48:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:10.78 +39:46:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:38.23 +37:37:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:48.95 +41:16:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:16.75 +37:59:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:06.01 +36:50:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:23.21 +40:36:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:31.98 +38:44:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.60 +36:56:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:22.88 +33:57:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:37.93 +41:48:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.02 +40:08:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:37.12 +36:25:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:39.28 +41:47:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:40.54 +37:18:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:07.66 +38:56:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:07.90 +39:15:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:13.37 +38:32:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.35 +40:55:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:47.47 +34:07:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:04.62 +37:45:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:13.83 +41:47:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.71 +39:46:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:58.72 +32:49:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:08.02 +36:40:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:31.85 +34:33:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:46.45 +39:39:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:05.43 +37:55:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:49.41 +33:25:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.47 +36:46:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:22.03 +33:37:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:09.55 +38:28:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:17.67 +39:47:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:36.78 +42:32:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:40.49 +40:49:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:48.84 +33:39:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:03.70 +34:22:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:37.01 +33:46:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:17.38 +34:47:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:30.92 +33:33:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:34.64 +41:55:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:55.87 +41:36:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:12.83 +33:36:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:21.30 +41:17:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:24.02 +42:26:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:24.82 +42:13:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:42.00 +36:19:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:14.11 +41:40:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:00.39 +33:22:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:52.17 +39:48:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:01.72 +41:06:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:21.93 +37:53:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:29.08 +33:18:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:41.50 +41:00:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:47.79 +41:23:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:05.70 +39:23:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:18.24 +34:10:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:28.17 +39:24:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:38.23 +42:04:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:17.79 +40:38:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:22.34 +40:13:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:23.97 +39:12:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:44.90 +40:34:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:48.54 +40:52:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:11.63 +39:57:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:29.73 +41:09:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:53.47 +39:12:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:16.88 +41:56:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:34.78 +39:09:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:36.85 +41:59:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:17.70 +41:28:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:25.90 +39:41:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:26.98 +40:50:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:53.29 +41:25:59.8 -- 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)
21:10:36.26 +40:19:47.7 -- not a known variable star
21:11:40.23 +34:59:54.3 -- not a known variable star
21:12:16.07 +34:09:55.3 -- not a known variable star
21:12:49.69 +41:23:26.1 -- a known variable star
21:13:42.11 +34:07:20.2 -- a known variable star
21:14:24.68 +33:06:52.2 -- not a known variable star
21:14:44.85 +38:12:02.9 -- not a known variable star
21:14:48.61 +37:08:04.4 -- not a known variable star
21:15:42.90 +33:53:34.2 -- not a known variable star
21:15:49.53 +38:27:47.2 -- a known variable star
21:16:29.73 +36:57:21.7 -- not a known variable star
21:16:59.17 +37:32:52.5 -- not a known variable star
21:17:23.18 +41:27:44.6 -- not a known variable star
21:17:37.36 +36:35:15.1 -- not a known variable star
21:17:44.37 +33:45:12.6 -- not a known variable star
21:18:35.07 +40:16:41.5 -- not a known variable star
21:20:25.20 +37:31:57.8 -- not a known variable star
21:20:52.04 +38:17:39.3 -- not a known variable star
21:21:02.46 +42:07:14.1 -- not a known variable star
21:21:47.75 +35:29:49.3 -- not a known variable star
21:24:39.60 +36:58:44.7 -- a known variable star
21:24:42.34 +38:26:37.6 -- a known variable star
21:25:05.40 +37:46:26.3 -- not a known variable star
21:26:25.15 +35:51:23.8 -- not a known variable star
21:27:07.29 +35:14:56.3 -- not a known variable star
21:27:59.53 +37:32:20.0 -- a known variable star
21:28:06.80 +39:56:16.2 -- a known variable star
21:28:08.25 +36:39:03.2 -- not a known variable star
21:29:05.00 +40:27:03.4 -- not a known variable star
21:29:07.94 +42:01:02.3 -- a known variable star
21:31:14.85 +38:46:29.2 -- a known variable star
21:31:28.72 +39:48:09.6 -- not a known variable star
21:33:10.78 +39:46:10.6 -- a known variable star
21:33:38.23 +37:37:16.6 -- not a known variable star
21:34:48.95 +41:16:17.1 -- not a known variable star
21:35:16.75 +37:59:46.9 -- not a known variable star
21:42:06.01 +36:50:53.5 -- not a known variable star
21:42:23.21 +40:36:52.9 -- not a known variable star
21:43:31.98 +38:44:13.9 -- not a known variable star
21:44:49.60 +36:56:52.9 -- not a known variable star
21:47:22.88 +33:57:51.4 -- a known variable star
21:48:37.93 +41:48:10.0 -- not a known variable star
21:48:47.02 +40:08:13.0 -- not a known variable star
21:54:37.12 +36:25:58.5 -- not a known variable star
21:57:39.28 +41:47:18.1 -- not a known variable star
21:57:40.54 +37:18:47.0 -- not a known variable star
21:58:07.66 +38:56:39.7 -- not a known variable star
22:01:07.90 +39:15:18.8 -- not a known variable star
22:01:13.37 +38:32:59.7 -- not a known variable star
22:01:22.35 +40:55:07.5 -- not a known variable star
22:01:47.47 +34:07:04.1 -- not a known variable star
22:02:04.62 +37:45:26.7 -- not a known variable star
22:02:13.83 +41:47:07.6 -- not a known variable star
22:03:59.71 +39:46:37.0 -- not a known variable star
22:04:58.72 +32:49:10.1 -- not a known variable star
22:05:08.02 +36:40:55.1 -- not a known variable star
22:06:31.85 +34:33:34.9 -- not a known variable star
22:06:46.45 +39:39:12.0 -- not a known variable star
22:07:05.43 +37:55:15.5 -- not a known variable star
22:07:49.41 +33:25:38.1 -- not a known variable star
22:09:11.47 +36:46:04.4 -- not a known variable star
22:12:22.03 +33:37:10.1 -- not a known variable star
22:14:09.55 +38:28:25.4 -- a known variable star
22:15:17.67 +39:47:52.8 -- not a known variable star
22:17:36.78 +42:32:37.0 -- not a known variable star
22:17:40.49 +40:49:15.2 -- not a known variable star
22:17:48.84 +33:39:27.3 -- not a known variable star
22:18:03.70 +34:22:51.4 -- not a known variable star
22:19:37.01 +33:46:32.0 -- not a known variable star
22:20:17.38 +34:47:25.5 -- not a known variable star
22:20:30.92 +33:33:33.5 -- a known variable star
22:20:34.64 +41:55:56.8 -- not a known variable star
22:20:55.87 +41:36:25.0 -- not a known variable star
22:21:12.83 +33:36:39.6 -- not a known variable star
22:21:21.30 +41:17:35.5 -- not a known variable star
22:21:24.02 +42:26:35.3 -- not a known variable star
22:21:24.82 +42:13:35.3 -- not a known variable star
22:21:42.00 +36:19:17.1 -- not a known variable star
22:22:14.11 +41:40:45.7 -- not a known variable star
22:23:00.39 +33:22:31.9 -- not a known variable star
22:23:52.17 +39:48:15.6 -- not a known variable star
22:24:01.72 +41:06:40.3 -- not a known variable star
22:24:21.93 +37:53:05.3 -- not a known variable star
22:24:29.08 +33:18:07.3 -- not a known variable star
22:24:41.50 +41:00:03.8 -- not a known variable star
22:24:47.79 +41:23:33.9 -- a known variable star
22:25:05.70 +39:23:43.0 -- not a known variable star
22:25:18.24 +34:10:33.3 -- not a known variable star
22:25:28.17 +39:24:20.4 -- not a known variable star
22:25:38.23 +42:04:06.0 -- not a known variable star
22:26:17.79 +40:38:19.1 -- not a known variable star
22:26:22.34 +40:13:20.2 -- not a known variable star
22:26:23.97 +39:12:20.6 -- a known variable star
22:26:44.90 +40:34:43.6 -- not a known variable star
22:26:48.54 +40:52:45.2 -- not a known variable star
22:27:11.63 +39:57:46.0 -- not a known variable star
22:27:29.73 +41:09:13.6 -- not a known variable star
22:27:53.47 +39:12:46.6 -- not a known variable star
22:28:16.88 +41:56:37.5 -- not a known variable star
22:28:34.78 +39:09:23.3 -- not a known variable star
22:28:36.85 +41:59:19.6 -- not a known variable star
22:29:17.70 +41:28:01.8 -- not a known variable star
22:29:25.90 +39:41:13.8 -- not a known variable star
22:29:26.98 +40:50:01.7 -- a known variable star
22:29:53.29 +41:25:59.8 -- not a known variable star
Found 89 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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105 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 105 (excluding asteroids and hot pixels, 89 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)2461177.94627731 -observatory V36
03:49:15.48 +20:41:58.9 Mercury (-2.1mag)
05:49:56.01 +24:57:39.0 Venus (-3.9mag)
01:47:03.55 +10:13:56.5 Mars (1.3mag)
07:31:27.43 +22:10:43.9 Jupiter (-1.9mag)
00:42:11.39 +02:07:51.7 Saturn (0.9mag)
03:54:56.63 +20:09:58.3 Uranus (5.8mag)
00:14:27.38 +00:06:57.9 Neptune (7.8mag)
20:34:09.74 -22:57:33.0 Pluto (14.5mag)
04:10:44.77 +25:17:56.5 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 362 May 17 08:03 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461177.94627731:
07:31:21.26 +22:10:59.4 Io (5.9mag)
07:31:20.43 +22:11:04.1 Europa (6.1mag)
07:31:10.86 +22:11:24.9 Ganymede (5.5mag)
07:31:49.24 +22:09:55.2 Callisto (6.7mag)
07:33:04.67 +21:48:09.0 Himalia (15.5mag)
07:31:28.71 +22:10:42.2 Thebe (16.4mag)
07:33:30.67 +22:12:58.6 Elara (17.4mag)
07:32:23.94 +22:34:10.4 Pasiphae (17.6mag)
07:38:53.68 +22:11:01.8 Carme (18.7mag)
00:42:14.59 +02:08:17.8 Titan (8.7mag)
00:42:08.05 +02:07:56.3 Rhea (10.0mag)
00:42:14.23 +02:06:31.1 Iapetus (11.4mag)
00:42:06.83 +02:07:36.1 Hyperion (14.7mag)
00:43:18.69 +02:12:50.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 17 08:03 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461177.94627731:
17:06:53.54 -31:12:21.1 JWST
19:59:57.92 -07:08:10.4 Chandra
23:31:37.31 +61:34:46.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 17 08:03 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461177.94627731 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
13:29:23.75 -27:55:45.9 14.5mag D/1884 O1 (Barnard)
06:22:22.90 +30:51:38.0 15.8mag D/1886 K1 (Brooks)
15:34:20.35 +00:52:34.4 14.7mag D/1895 Q1 (Swift)
05:14:11.71 +24:17:54.2 17.1mag D/1918 W1 (Schorr)
08:27:39.25 +21:52:28.1 17.7mag P/2009 WX51 (Catalina)
18:54:13.64 -30:58:10.0 13.7mag P/2010 H2 (Vales)
05:32:44.54 -68:28:34.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:41:20.84 +31:42:41.7 17.4mag C/2017 K2 (PANSTARRS)
17:23:02.62 +13:51:03.8 17.7mag C/2021 G2 (ATLAS)
23:14:49.69 +30:38:43.2 17.2mag C/2022 E2 (ATLAS)
05:07:13.28 +26:44:04.2 16.3mag C/2022 N2 (PANSTARRS)
09:15:48.46 +31:42:53.7 16.5mag C/2022 QE78 (ATLAS)
08:40:11.20 +02:38:14.9 17.5mag C/2022 R6 (PANSTARRS)
18:41:18.22 +20:47:04.5 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:28:09.34 -11:06:17.4 17.5mag P/2023 B1 (PANSTARRS)
08:59:48.97 -07:35:33.9 17.9mag C/2023 F3 (ATLAS)
22:14:45.87 +65:02:13.2 17.7mag C/2023 H5 (Lemmon)
18:35:18.89 -04:54:58.1 13.8mag C/2023 R1 (PANSTARRS)
14:34:52.62 +87:24:00.8 17.9mag C/2023 X2 (Lemmon)
06:43:19.20 +63:44:15.5 17.5mag C/2024 A1 (ATLAS)
06:12:27.08 +25:19:28.2 12.8mag C/2024 E1 (Wierzchos)
15:55:12.39 +11:08:16.5 17.3mag C/2024 G6 (ATLAS)
20:22:22.95 +24:28:50.9 14.2mag C/2024 J3 (ATLAS)
03:56:17.44 -18:09:57.0 16.2mag C/2024 T5 (ATLAS)
05:45:23.27 +38:27:32.4 17.9mag C/2025 J1 (Borisov)
11:59:03.43 +53:24:10.3 16.6mag C/2025 L1 (ATLAS)
06:02:26.19 -09:15:05.5 11.4mag C/2025 R3 (PANSTARRS)
12:42:46.34 +04:26:09.4 17.2mag C/2025 Y1 (ATLAS)
01:18:05.87 +41:33:13.3 15.5mag C/2026 B2 (Sun-Gao)
11:12:09.87 -13:17:52.9 16.1mag A/2026 E1
19:43:17.63 -08:13:41.8 10.0mag 10P/Tempel
14:23:55.74 -01:09:49.6 16.9mag 24P/Schaumasse
10:59:03.72 -00:53:14.9 15.9mag 29P/Schwassmann-Wachmann
10:46:02.62 -02:37:12.5 17.6mag 43P/Wolf-Harrington
02:37:47.02 +22:32:56.0 17.5mag 47P/Ashbrook-Jackson
08:13:45.98 +29:39:06.3 16.9mag 63P/Wild
00:05:56.31 -08:04:56.2 15.7mag 65P/Gunn
05:34:16.42 +30:02:24.4 16.3mag 76P/West-Kohoutek-Ikemura
02:17:19.18 +14:00:00.8 14.0mag 78P/Gehrels
00:29:49.61 -00:25:01.2 15.1mag 88P/Howell
03:44:59.48 +27:37:36.1 15.1mag 93P/Lovas
06:00:07.73 +33:19:24.1 15.8mag 123P/West-Hartley
09:13:34.84 +24:06:48.4 16.4mag 124P/Mrkos
03:23:18.70 +17:32:57.0 16.4mag 128P/Shoemaker-Holt
03:50:04.19 +17:42:14.3 17.7mag 131P/Mueller
04:14:53.61 +19:35:05.7 12.0mag 141P/Machholz
04:18:18.70 +14:47:06.2 11.9mag 141P-A/Machholz
02:59:55.57 +11:23:16.1 10.5mag 141P-D/Machholz
02:41:36.63 -28:07:40.8 17.6mag 161P/Hartley-IRAS
02:33:06.57 +14:09:38.3 14.8mag 162P/SidingSpring
19:30:54.04 -03:39:45.0 18.0mag 169P/NEAT
17:08:38.22 -10:11:28.2 16.2mag 235P/LINEAR
06:45:02.25 +35:55:07.0 17.2mag 240P/NEAT
23:36:10.88 -11:03:41.1 17.0mag 260P/McNaught
03:08:17.28 +28:01:26.1 17.7mag 295P/LINEAR
15:26:35.41 +08:19:37.7 17.4mag 391P/Kowalski
07:51:07.28 +21:11:03.6 17.8mag 450P/LONEOS
06:24:36.68 +43:09:03.1 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 17 08:03 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
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
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
01:13:11.60 -33:25:16.10 2026-05-13.41 16.8
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
01:13:11.60 -33:25:16.10 2026-05-13.41 16.8
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
-rw-r--r-- 1 apache apache 5.8K May 17 08:03 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
-rw-r--r-- 1 apache apache 188K May 17 08:03 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:34:26.500 +54:57:10.77 AT 2026mec 2026-05-02.78 21.1
12:14:27.750 +34:57:43.97 AT 2026meb 2026-05-02.77 20.34
17:58:41.940 +24:07:46.04 AT 2026mea 2026-05-01.81 20.94
12:12:11.350 +37:58:49.88 AT 2026mdz 2026-04-28.85 20.98
12:08:07.370 +51:57:57.83 AT 2026mdy 2026-04-28.84 21.16
12:38:44.690 +53:19:33.47 AT 2026mdx 2026-04-28.84 21.35
18:21:55.260 +43:11:30.40 AT 2026mdw 2026-04-27.88 21.86
18:21:07.200 +32:13:29.52 AT 2026mdv 2026-04-24.76 20.8
11:41:38.770 +41:26:21.55 AT 2026mdu 2026-04-23.84 21.32
18:15:31.440 +39:24:49.52 AT 2026mdt 2026-04-22.78 21.22
18:17:34.880 +35:01:54.50 AT 2026mds 2026-04-22.77 19.98
18:14:32.100 +33:04:52.93 AT 2026mdr 2026-04-22.77 20.46
14:26:56.430 +05:21:18.75 AT 2026mdq 2026-05-09.69 22.12
14:28:31.360 -01:19:36.91 AT 2026mdp 2026-05-09.69 22.45
14:25:04.120 +03:58:59.69 AT 2026mdo 2026-05-09.69 22.57
14:12:45.800 +05:24:46.71 AT 2026mdn 2026-05-09.69 22.42
13:47:08.710 +03:21:10.28 AT 2026mdm 2026-05-09.68 22.03
13:37:42.620 +02:27:43.78 AT 2026mdl 2026-05-09.68 22.57
13:24:50.420 +03:27:16.10 AT 2026mdk 2026-05-09.67 22.21
13:13:43.170 +00:51:15.49 AT 2026mdj 2026-05-09.67 22.15
-rw-r--r-- 1 apache apache 30K May 17 08:03 tns_transients_list.txt
