This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m
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 19.2895 2461179.7895 11.55 21:44:38.58 +38:02:24.8
87.13219 -11.52186 galactic Cyg Second-epoch detections are separated by 2.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:38.58 +38:02:24.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.665+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:38.58 +38:02:24.8: 12.94 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:38.58 +38:02:24.8: 14.01 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461179.7895,11.55,0.05,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 20260519.2895 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.75 21:23:29.50 +39:22:20.0
85.00663 -7.72651 galactic Cyg Second-epoch detections are separated by 2.1" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:23:29.50 +39:22:20.0 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:29.50 +39:22:20.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:29.50 +39:22:20.0: 13.91 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461179.7895,11.75,0.05,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 20260519.2895 11.75CV 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 19.2895 2461179.7895 11.46 21:55:57.21 +40:10:26.6
90.24660 -11.30742 galactic Cyg Second-epoch detections are separated by 3.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9858+40.1754 | 21:55:57.21 +40:10:26.6 (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 21:55:57.21 +40:10:26.6: 13.26 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:57.21 +40:10:26.6: 13.81 +/- 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 J328.9858+40.1754,2461179.7895,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9858+40.1754 20260519.2895 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.56 21:10:17.90 +39:56:34.8
83.65098 -5.49947 galactic Cyg Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:17.90 +39:56:34.8 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:17.90 +39:56:34.8: 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 21:10:17.90 +39:56:34.8: 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
target,2461179.7895,11.56,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.60 21:14:56.94 +37:19:03.4
82.34082 -7.95395 galactic Cyg Second-epoch detections are separated by 2.1" and 1.2 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 | 21:14:56.94 +37:19:03.4 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:56.94 +37:19:03.4: 13.16 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:56.94 +37:19:03.4: 13.88 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461179.7895,11.60,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.37 22:01:22.40 +40:55:09.3
91.54159 -11.36319 galactic Lac Second-epoch detections are separated by 0.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3389+40.9153 | 22:01:22.40 +40:55:09.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.776+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.40 +40:55:09.3: 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 22:01:22.40 +40:55:09.3: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 J330.3389+40.9153,2461179.7895,11.37,0.05,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 J330.3389+40.9153 20260519.2895 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 19.2895 2461179.7895 11.47 21:32:27.21 +38:28:54.9
85.63984 -9.58079 galactic Cyg Second-epoch detections are separated by 1.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1964311887063133440 | 21:32:26.35 +38:28:21.4 (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 21:32:27.21 +38:28:54.9: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:27.21 +38:28:54.9: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 1964311887063133440,2461179.7895,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964311887063133440 20260519.2895 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.62 21:36:54.23 +40:36:46.5
87.74736 -8.60798 galactic Cyg Second-epoch detections are separated by 0.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2332+40.6116 | 21:36:54.23 +40:36:46.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.644+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:54.23 +40:36:46.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:54.23 +40:36:46.5: 14.06 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 J324.2332+40.6116,2461179.7895,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2332+40.6116 20260519.2895 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.61 21:17:09.32 +42:14:59.2
86.22529 -4.85426 galactic Cyg Second-epoch detections are separated by 2.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.2878+42.2484 | 21:17:09.32 +42:14:59.2 (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 21:17:09.32 +42:14:59.2: 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 21:17:09.32 +42:14:59.2: 13.87 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 J319.2878+42.2484,2461179.7895,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.2878+42.2484 20260519.2895 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.34 21:42:55.18 +37:35:20.8
86.56673 -11.63355 galactic Cyg Second-epoch detections are separated by 0.7" and 1.4 pix
The object was found in VSX25" Gaia DR3 1952713070181680896
Type: VAR
# Max. Min./Amp. JD0 Period
15.110 G 15.330 G 0.025300400000 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 21:42:55.18 +37:35:20.8: 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 21:42:55.18 +37:35:20.8: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 1952713070181680896,2461179.7895,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952713070181680896 20260519.2895 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 19.2895 2461179.7895 11.28 21:23:18.20 +42:11:40.3
86.98850 -5.70339 galactic Cyg Second-epoch detections are separated by 4.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.8337+42.1953 | 21:23:18.20 +42:11:40.3 (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 21:23:18.20 +42:11:40.3: 13.35 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:18.20 +42:11:40.3: 13.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 J320.8337+42.1953,2461179.7895,11.28,0.05,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 J320.8337+42.1953 20260519.2895 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 19.2895 2461179.7895 11.34 21:20:22.07 +36:42:26.0
82.65036 -9.15770 galactic Cyg Second-epoch detections are separated by 1.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.0976+36.7086 | 21:20:22.07 +36:42:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.720+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:22.07 +36:42:26.0: 11.75 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:22.07 +36:42:26.0: 13.56 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J320.0976+36.7086,2461179.7895,11.34,0.05,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 J320.0976+36.7086 20260519.2895 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 19.2895 2461179.7895 11.36 21:17:45.95 +35:45:18.2
81.58623 -9.43898 galactic Cyg Second-epoch detections are separated by 0.9" and 1.6 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 | 21:17:45.95 +35:45:18.2 (user input) | T | P | (position from user input) J-Ks=0.239+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:45.95 +35:45:18.2: 12.42 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:45.95 +35:45:18.2: 13.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.23 +/- 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,2461179.7895,11.36,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.02 21:34:37.49 +34:15:56.5
82.99630 -12.93453 galactic Cyg Second-epoch detections are separated by 1.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:37.49 +34:15:56.5 (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 21:34:37.49 +34:15:56.5: 12.90 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:37.49 +34:15:56.5: 13.28 +/- 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
target,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.23 21:10:10.05 +42:07:59.7
85.24794 -3.99444 galactic Cyg Second-epoch detections are separated by 0.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.5422+42.1347 | 21:10:10.05 +42:07:59.7 (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 21:10:10.05 +42:07:59.7: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:10.05 +42:07:59.7: 13.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 J317.5422+42.1347,2461179.7895,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.5422+42.1347 20260519.2895 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 19.2895 2461179.7895 11.13 21:48:47.05 +40:08:13.9
89.14873 -10.46152 galactic Cyg Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 21:48:47.05 +40:08:13.9: 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 21:48:47.05 +40:08:13.9: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 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+40.1375,2461179.7895,11.13,0.05,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 J327.1964+40.1375 20260519.2895 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 19.2895 2461179.7895 11.30 21:15:25.75 +36:10:50.0
81.57031 -8.80311 galactic Cyg Second-epoch detections are separated by 2.5" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.8553+36.1819 | 21:15:25.75 +36:10:50.0 (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 21:15:25.75 +36:10:50.0: 12.89 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:25.75 +36:10:50.0: 13.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 J318.8553+36.1819,2461179.7895,11.30,0.05,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
ATO J318.8553+36.1819 20260519.2895 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 19.2895 2461179.7895 10.81 22:14:40.29 +33:58:19.1
89.38643 -18.49603 galactic Peg Second-epoch detections are separated by 2.1" and 1.2 pix
The object was found in VSX21" Gaia DR3 1905375452470197632
Type: RS
# Max. Min./Amp. JD0 Period
14.710 G 14.820 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 22:14:40.29 +33:58:19.1: 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 22:14:40.29 +33:58:19.1: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 1905375452470197632,2461179.7895,10.81,0.05,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
Gaia DR3 1905375452470197632 20260519.2895 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 19.2895 2461179.7895 11.22 21:40:56.21 +41:13:24.8
88.73322 -8.66556 galactic Cyg Second-epoch detections are separated by 0.5" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2343+41.2229 | 21:40:56.21 +41:13:24.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.331+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:56.21 +41:13:24.8: 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 21:40:56.21 +41:13:24.8: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2343+41.2229,2461179.7895,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2343+41.2229 20260519.2895 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.24 21:12:34.00 +38:29:35.1
82.88205 -6.80745 galactic Cyg Second-epoch detections are separated by 0.3" and 1.3 pix
The object was found in VSX 6" Gaia DR3 1965052339423436288
Type: S
# Max. Min./Amp. JD0 Period
16.780 G 17.180 G 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 21:12:34.00 +38:29:35.1: 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 21:12:34.00 +38:29:35.1: 13.44 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 1965052339423436288,2461179.7895,11.24,0.05,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 1965052339423436288 20260519.2895 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 19.2895 2461179.7895 10.95 21:32:55.76 +38:02:35.9
85.40208 -9.96316 galactic Cyg Second-epoch detections are separated by 0.1" and 1.4 pix
The object was found in VSX18" Gaia DR3 1952257013374510336
Type: ROT
# Max. Min./Amp. JD0 Period
12.510 G 12.540 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 21:32:55.76 +38:02:35.9: 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 21:32:55.76 +38:02:35.9: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952257013374510336,2461179.7895,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952257013374510336 20260519.2895 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 19.2895 2461179.7895 10.77 22:05:39.71 +34:53:40.0
88.41774 -16.63885 galactic Peg Second-epoch detections are separated by 1.6" and 1.5 pix
The object was found in VSX18" Gaia DR3 1900468744392395008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.160 G 13.190 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 22:05:39.71 +34:53:40.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:39.71 +34:53:40.0: 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 1900468744392395008,2461179.7895,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1900468744392395008 20260519.2895 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.02 21:18:51.01 +34:56:41.1
81.14568 -10.15803 galactic Cyg Second-epoch detections are separated by 0.7" and 1.6 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 J319.7197+34.9474 | 21:18:52.73 +34:56:50.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.027 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:51.01 +34:56:41.1: 11.94 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:51.01 +34:56:41.1: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J319.7197+34.9474,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.7197+34.9474 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.95 21:27:23.91 +33:39:59.0
81.46967 -12.31422 galactic Cyg Second-epoch detections are separated by 1.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1854304305596960256 | 21:27:21.99 +33:40:12.4 (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 21:27:23.91 +33:39:59.0: 11.07 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:23.91 +33:39:59.0: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.03 +/- 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 1854304305596960256,2461179.7895,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1854304305596960256 20260519.2895 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 19.2895 2461179.7895 11.11 21:23:28.52 +42:28:11.4
87.20613 -5.53049 galactic Cyg Second-epoch detections are separated by 0.6" and 1.2 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 J320.8752+42.4723 | 21:23:30.88 +42:28:19.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:28.52 +42:28:11.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:28.52 +42:28:11.4: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 J320.8752+42.4723,2461179.7895,11.11,0.05,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 J320.8752+42.4723 20260519.2895 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 19.2895 2461179.7895 10.88 21:41:19.29 +37:02:32.5
85.95212 -11.82789 galactic Cyg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:19.29 +37:02:32.5 (user input) | T | P | (position from user input) J-Ks=0.669+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:19.29 +37:02:32.5: 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 21:41:19.29 +37:02:32.5: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461179.7895,10.88,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.62 21:34:48.59 +33:48:32.7
82.70050 -13.29086 galactic Cyg Second-epoch detections are separated by 0.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950175225548790528 | 21:34:51.66 +33:48:08.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.612+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:48.59 +33:48:32.7: 11.51 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:48.59 +33:48:32.7: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 1950175225548790528,2461179.7895,10.62,0.05,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
Gaia DR3 1950175225548790528 20260519.2895 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 19.2895 2461179.7895 10.91 21:17:20.43 +36:43:55.1
82.24281 -8.70322 galactic Cyg Second-epoch detections are separated by 2.1" and 1.1 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 J319.3393+36.7289 | 21:17:20.43 +36:43:55.1 (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 21:17:20.43 +36:43:55.1: 11.64 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:20.43 +36:43:55.1: 12.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 J319.3393+36.7289,2461179.7895,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3393+36.7289 20260519.2895 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.51 21:32:51.75 +35:15:27.0
83.43195 -11.96824 galactic Cyg Second-epoch detections are separated by 1.3" and 1.6 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 J323.2165+35.2577 | 21:32:51.75 +35:15:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:51.75 +35:15:27.0: 13.33 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:51.75 +35:15:27.0: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.2165+35.2577,2461179.7895,10.51,0.05,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 J323.2165+35.2577 20260519.2895 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 19.2895 2461179.7895 10.76 21:20:25.16 +37:31:58.3
83.25686 -8.58963 galactic Cyg Second-epoch detections are separated by 0.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.1010+37.5280 | 21:20:25.16 +37:31:58.3 (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 21:20:25.16 +37:31:58.3: 11.43 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:25.16 +37:31:58.3: 12.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.46 +/- 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+37.5280,2461179.7895,10.76,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.79 21:11:48.56 +37:16:05.0
81.87446 -7.53107 galactic Cyg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:11:48.56 +37:16:05.0 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:48.56 +37:16:05.0: 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 21:11:48.56 +37:16:05.0: 12.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.70 +/- 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,2461179.7895,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.44 21:28:11.80 +34:45:27.9
82.37698 -11.65802 galactic Cyg Second-epoch detections are separated by 2.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:11.80 +34:45:27.9 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:11.80 +34:45:27.9: 10.69 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.80 +34:45:27.9: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461179.7895,10.44,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.62 21:21:12.47 +36:20:38.0
82.50549 -9.53194 galactic Cyg Second-epoch detections are separated by 0.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1963647331061827072 | 21:21:10.96 +36:20:33.5 (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 21:21:12.47 +36:20:38.0: 11.35 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:12.47 +36:20:38.0: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 1963647331061827072,2461179.7895,10.62,0.05,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
Gaia DR3 1963647331061827072 20260519.2895 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 19.2895 2461179.7895 10.38 21:22:57.41 +34:56:38.4
81.73966 -10.76388 galactic Cyg Second-epoch detections are separated by 3.8" and 1.7 pix
The object was found in VSX16" Gaia DR3 1855400308227023616
Type: ROT
# Max. Min./Amp. JD0 Period
12.260 G 12.290 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 21:22:57.41 +34:56:38.4: 10.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:57.41 +34:56:38.4: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855400308227023616,2461179.7895,10.38,0.05,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
Gaia DR3 1855400308227023616 20260519.2895 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 19.2895 2461179.7895 9.85 22:13:23.24 +33:35:20.4
88.91973 -18.64489 galactic Peg Second-epoch detections are separated by 0.9" and 1.6 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 1899358649965242624 | 22:13:25.31 +33:35:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.329+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:13:23.24 +33:35:20.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:13:23.24 +33:35:20.4: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1899358649965242624,2461179.7895,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899358649965242624 20260519.2895 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.15 21:35:00.60 +35:11:24.6
83.70866 -12.31995 galactic Cyg Second-epoch detections are separated by 1.2" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.7527+35.1912 | 21:34:59.56 +35:11:10.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:00.60 +35:11:24.6: 12.77 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:00.60 +35:11:24.6: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.7527+35.1912,2461179.7895,10.15,0.05,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
ATO J323.7527+35.1912 20260519.2895 10.15CV 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 19.2895 2461179.7895 10.18 21:19:48.16 +37:09:11.9
82.89504 -8.76612 galactic Cyg Second-epoch detections are separated by 0.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.9489+37.1625 | 21:19:46.85 +37:09:11.4 (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 21:19:48.16 +37:09:11.9: 11.02 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:48.16 +37:09:11.9: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J319.9489+37.1625,2461179.7895,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.9489+37.1625 20260519.2895 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.36 22:00:18.66 +38:06:30.6
89.59951 -13.44768 galactic Lac Second-epoch detections are separated by 4.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.0789+38.1088 | 22:00:18.96 +38:06:31.8 (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 22:00:18.66 +38:06:30.6: 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 22:00:18.66 +38:06:30.6: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.0789+38.1088,2461179.7895,9.36,0.05,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 J330.0789+38.1088 20260519.2895 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 19.2895 2461179.7895 9.60 22:01:18.64 +41:30:28.5
91.89991 -10.89090 galactic Lac Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959759393525967360 | 22:01:19.91 +41:30:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.219+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:18.64 +41:30:28.5: 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 22:01:18.64 +41:30:28.5: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959759393525967360,2461179.7895,9.60,0.05,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
Gaia DR3 1959759393525967360 20260519.2895 9.60CV 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 19.2895 2461179.7895 9.48 22:12:38.32 +38:19:17.8
91.72044 -14.74265 galactic Lac Second-epoch detections are separated by 1.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.1591+38.3114 | 22:12:39.69 +38:19:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.679+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:38.32 +38:19:17.8: 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 22:12:38.32 +38:19:17.8: 11.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.1591+38.3114,2461179.7895,9.48,0.05,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 J333.1591+38.3114 20260519.2895 9.48CV 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 19.2895 2461179.7895 7.08 22:22:38.66 +33:28:06.7
90.50249 -19.87111 galactic Peg Second-epoch detections are separated by 0.7" and 1.5 pix
The object was found in VSX 7" Gaia DR3 1902157525533110272
Type: ROT
# Max. Min./Amp. JD0 Period
10.330 G 10.380 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 22:22:38.66 +33:28:06.7: 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 22:22:38.66 +33:28:06.7: 9.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.99 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902157525533110272,2461179.7895,7.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902157525533110272 20260519.2895 7.08CV 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 19.2895 2461179.7895 7.34 22:19:05.13 +32:54:15.2
89.50950 -19.90120 galactic Peg Second-epoch detections are separated by 1.1" and 1.5 pix
The object was found in VSX 1" Gaia DR3 1905024914419924608
Type: ACV|roAm|
# Max. Min./Amp. JD0 Period
9.360 G 9.390 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 22:19:05.13 +32:54:15.2: 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 22:19:05.13 +32:54:15.2: 10.16 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.16 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1905024914419924608,2461179.7895,7.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905024914419924608 20260519.2895 7.34CV 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 19.2895 2461179.7895 7.47 22:22:02.85 +32:44:45.0
89.95162 -20.39111 galactic Peg Second-epoch detections are separated by 0.7" and 1.6 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 1901983768335969536 | 22:22:02.65 +32:44:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:02.85 +32:44:45.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:02.85 +32:44:45.0: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.50 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901983768335969536,2461179.7895,7.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901983768335969536 20260519.2895 7.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 7.64 22:22:13.30 +32:50:51.7
90.04608 -20.32888 galactic Peg Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901986104798328704 | 22:22:13.14 +32:50:53.9 (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 22:22:13.30 +32:50:51.7: 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 22:22:13.30 +32:50:51.7: 10.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901986104798328704,2461179.7895,7.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901986104798328704 20260519.2895 7.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 7.97 22:01:07.87 +39:15:18.6
90.45748 -12.64651 galactic Lac Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 22:01:07.87 +39:15:18.6: 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 22:01:07.87 +39:15:18.6: 10.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.24 +/- 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 108695,2461179.7895,7.97,0.05,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
HIP 108695 20260519.2895 7.97CV 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 19.2895 2461179.7895 7.80 22:18:24.32 +32:54:23.2
89.38776 -19.81590 galactic Peg Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905027079082530048 | 22:18:24.37 +32:54:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.544+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:24.32 +32:54:23.2: 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 22:18:24.32 +32:54:23.2: 10.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1905027079082530048,2461179.7895,7.80,0.05,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 1905027079082530048 20260519.2895 7.80CV 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 19.2895 2461179.7895 7.84 22:21:28.71 +32:41:44.2
89.81643 -20.36309 galactic Peg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901960644232046080 | 22:21:28.59 +32:41:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.665+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:28.71 +32:41:44.2: 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 22:21:28.71 +32:41:44.2: 10.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901960644232046080,2461179.7895,7.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901960644232046080 20260519.2895 7.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 7.96 22:23:54.63 +33:02:50.9
90.47790 -20.36792 galactic Peg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902085335722026240 | 22:23:54.55 +33:02:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=0.644+/-9.995 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:54.63 +33:02:50.9: 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 22:23:54.63 +33:02:50.9: 10.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902085335722026240,2461179.7895,7.96,0.05,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 1902085335722026240 20260519.2895 7.96CV 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 19.2895 2461179.7895 8.10 22:24:12.27 +32:53:19.9
90.43557 -20.53341 galactic Peg Second-epoch detections are separated by 1.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902068671249717376 | 22:24:12.14 +32:53:22.1 (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 22:24:12.27 +32:53:19.9: 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 22:24:12.27 +32:53:19.9: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902068671249717376,2461179.7895,8.10,0.05,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
Gaia DR3 1902068671249717376 20260519.2895 8.10CV 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 19.2895 2461179.7895 8.29 22:19:19.12 +32:44:18.3
89.44882 -20.06441 galactic Peg Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902015929050769792 | 22:19:19.27 +32:44:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.997+/-0.029 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:19.12 +32:44:18.3: 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 22:19:19.12 +32:44:18.3: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902015929050769792,2461179.7895,8.29,0.05,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 1902015929050769792 20260519.2895 8.29CV 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 19.2895 2461179.7895 8.52 22:22:13.07 +32:41:36.1
89.95063 -20.45464 galactic Peg Second-epoch detections are separated by 0.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901979679527114624 | 22:22:12.88 +32:41:38.9 (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 22:22:13.07 +32:41:36.1: 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 22:22:13.07 +32:41:36.1: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901979679527114624,2461179.7895,8.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901979679527114624 20260519.2895 8.52CV 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 19.2895 2461179.7895 8.62 22:21:18.80 +32:47:18.4
89.84341 -20.26726 galactic Peg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902008610427489280 | 22:21:18.62 +32:47:21.3 (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 22:21:18.80 +32:47:18.4: 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 22:21:18.80 +32:47:18.4: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902008610427489280,2461179.7895,8.62,0.05,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
Gaia DR3 1902008610427489280 20260519.2895 8.62CV 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 19.2895 2461179.7895 8.69 22:23:43.93 +33:23:34.1
90.65481 -20.06282 galactic Peg Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902146770934324352 | 22:23:43.91 +33:23:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.619+/-0.022 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:43.93 +33:23:34.1: 11.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:43.93 +33:23:34.1: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902146770934324352,2461179.7895,8.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902146770934324352 20260519.2895 8.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 8.69 22:24:02.20 +32:39:09.6
90.26075 -20.70737 galactic Peg Second-epoch detections are separated by 1.0" and 1.7 pix
The object was found in VSX25" Gaia DR3 1901783038741868288
Type: S
# Max. Min./Amp. JD0 Period
17.090 G 18.070 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 22:24:02.20 +32:39:09.6: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:02.20 +32:39:09.6: 11.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901783038741868288,2461179.7895,8.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901783038741868288 20260519.2895 8.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 8.71 22:20:07.11 +32:50:48.7
89.66154 -20.07417 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902023488194156288 | 22:20:07.25 +32:50:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.683+/-0.054 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:07.11 +32:50:48.7: 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 22:20:07.11 +32:50:48.7: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902023488194156288,2461179.7895,8.71,0.05,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 1902023488194156288 20260519.2895 8.71CV 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 19.2895 2461179.7895 8.81 22:24:47.50 +33:40:33.0
91.01918 -19.95499 galactic Peg Second-epoch detections are separated by 0.6" and 1.6 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 1902175736194553216 | 22:24:47.68 +33:40:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:47.50 +33:40:33.0: 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 22:24:47.50 +33:40:33.0: 11.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902175736194553216,2461179.7895,8.81,0.05,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
Gaia DR3 1902175736194553216 20260519.2895 8.81CV 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 19.2895 2461179.7895 8.90 22:20:30.33 +32:41:34.8
89.63688 -20.24666 galactic Peg Second-epoch detections are separated by 0.7" and 1.5 pix
The object was found in ASASSN-V 2" ASASSN-V J222030.45+324133.8
Type: SR
MeanMag 11.69 m Amp. 0.09 m Period 16.3366038 d
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 22:20:30.33 +32:41:34.8: 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 22:20:30.33 +32:41:34.8: 11.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461179.7895,8.90,0.05,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
VARIABLE_NAME 20260519.2895 8.90CV 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 19.2895 2461179.7895 9.48 21:31:14.81 +38:46:29.9
85.67190 -9.20607 galactic Cyg Second-epoch detections are separated by 1.0" and 1.3 pix
The object was found in VSX 3" 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 21:31:14.81 +38:46:29.9: 12.59 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:14.81 +38:46:29.9: 12.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461179.7895,9.48,0.05,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
V2072 Cyg 20260519.2895 9.48CV 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 19.2895 2461179.7895 9.05 22:18:11.58 +32:43:33.2
89.23676 -19.93601 galactic Peg Second-epoch detections are separated by 0.8" and 1.6 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 1899015945935483008 | 22:18:11.64 +32:43:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:11.58 +32:43:33.2: 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 22:18:11.58 +32:43:33.2: 12.03 +/- 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
Gaia DR3 1899015945935483008,2461179.7895,9.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899015945935483008 20260519.2895 9.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.01 22:23:12.48 +33:23:24.9
90.55757 -20.00255 galactic Peg Second-epoch detections are separated by 1.6" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902141754412380416 | 22:23:12.47 +33:23:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.999+/-0.025 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:12.48 +33:23:24.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:12.48 +33:23:24.9: 12.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902141754412380416,2461179.7895,9.01,0.05,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 1902141754412380416 20260519.2895 9.01CV 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 19.2895 2461179.7895 9.05 22:24:20.54 +32:49:58.8
90.42702 -20.59581 galactic Peg Second-epoch detections are separated by 1.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902067468658102912 | 22:24:20.43 +32:50:01.6 (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 22:24:20.54 +32:49:58.8: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:20.54 +32:49:58.8: 12.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902067468658102912,2461179.7895,9.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902067468658102912 20260519.2895 9.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.12 22:20:10.09 +32:56:33.4
89.72978 -20.00229 galactic Peg Second-epoch detections are separated by 0.4" and 1.6 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 1902025240539967488 | 22:20:10.22 +32:56:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.657+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:10.09 +32:56:33.4: 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 22:20:10.09 +32:56:33.4: 12.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902025240539967488,2461179.7895,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902025240539967488 20260519.2895 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.18 22:23:08.16 +32:50:44.2
90.21258 -20.44080 galactic Peg Second-epoch detections are separated by 1.4" and 1.6 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 1901988544339885056 | 22:23:07.99 +32:50:47.2 (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 22:23:08.16 +32:50:44.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:08.16 +32:50:44.2: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901988544339885056,2461179.7895,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901988544339885056 20260519.2895 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.16 22:22:11.78 +32:41:01.7
89.94081 -20.45985 galactic Peg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901979679527114624 | 22:22:12.88 +32:41:38.9 (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 22:22:11.78 +32:41:01.7: 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 22:22:11.78 +32:41:01.7: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901979679527114624,2461179.7895,9.16,0.05,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 1901979679527114624 20260519.2895 9.16CV 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 19.2895 2461179.7895 9.28 22:29:53.30 +41:26:00.2
96.34888 -14.01817 galactic Lac Second-epoch detections are separated by 1.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 22:29:53.30 +41:26:00.2: 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 22:29:53.30 +41:26:00.2: 12.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 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+41.4238,2461179.7895,9.28,0.05,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 J337.4722+41.4238 20260519.2895 9.28CV 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 19.2895 2461179.7895 9.20 22:23:07.72 +33:37:19.1
90.68372 -19.80281 galactic Peg Second-epoch detections are separated by 1.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902164947235888384 | 22:23:07.66 +33:37:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.755+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:07.72 +33:37:19.1: 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 22:23:07.72 +33:37:19.1: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902164947235888384,2461179.7895,9.20,0.05,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
Gaia DR3 1902164947235888384 20260519.2895 9.20CV 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 19.2895 2461179.7895 9.20 22:20:46.87 +32:50:51.1
89.78267 -20.15438 galactic Peg Second-epoch detections are separated by 0.8" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902012561796532608 | 22:20:47.03 +32:50:50.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.958+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:46.87 +32:50:51.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:46.87 +32:50:51.1: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902012561796532608,2461179.7895,9.20,0.05,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
Gaia DR3 1902012561796532608 20260519.2895 9.20CV 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 19.2895 2461179.7895 9.29 22:18:46.75 +32:43:54.8
89.34677 -20.00340 galactic Peg Second-epoch detections are separated by 0.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1896014932023521536 | 22:18:46.82 +32:43:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.177+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:46.75 +32:43:54.8: 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 22:18:46.75 +32:43:54.8: 12.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1896014932023521536,2461179.7895,9.29,0.05,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 1896014932023521536 20260519.2895 9.29CV 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 19.2895 2461179.7895 9.99 21:15:17.39 +38:56:43.9
83.58049 -6.88460 galactic Cyg Second-epoch detections are separated by 1.6" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.8439+38.9431 | 21:15:19.94 +38:56:57.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:17.39 +38:56:43.9: 11.62 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:17.39 +38:56:43.9: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J318.8439+38.9431,2461179.7895,9.99,0.05,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 J318.8439+38.9431 20260519.2895 9.99CV 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 19.2895 2461179.7895 9.31 22:23:11.20 +32:49:39.7
90.21094 -20.46158 galactic Peg Second-epoch detections are separated by 0.6" and 1.6 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 1901976346632766976 | 22:23:11.06 +32:49:42.1 (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 22:23:11.20 +32:49:39.7: 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 22:23:11.20 +32:49:39.7: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 1901976346632766976,2461179.7895,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901976346632766976 20260519.2895 9.31CV 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 19.2895 2461179.7895 9.38 22:25:10.70 +33:50:28.1
91.18899 -19.86392 galactic Peg Second-epoch detections are separated by 1.0" and 1.3 pix
The object was found in VSX 2" Gaia DR3 1902183398415669120
Type: ROT
# Max. Min./Amp. JD0 Period
11.330 G 11.370 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 22:25:10.70 +33:50:28.1: 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 22:25:10.70 +33:50:28.1: 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 1902183398415669120,2461179.7895,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902183398415669120 20260519.2895 9.38CV 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 19.2895 2461179.7895 9.38 22:23:49.51 +33:28:26.0
90.72090 -20.00718 galactic Peg Second-epoch detections are separated by 1.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902149622792600192 | 22:23:49.52 +33:28:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.642+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:49.51 +33:28:26.0: 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 22:23:49.51 +33:28:26.0: 12.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 1902149622792600192,2461179.7895,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902149622792600192 20260519.2895 9.38CV 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 19.2895 2461179.7895 9.35 22:24:41.55 +33:06:45.4
90.66117 -20.40746 galactic Peg Second-epoch detections are separated by 0.9" and 1.6 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 1902080662798445696 | 22:24:41.51 +33:06:48.0 (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 22:24:41.55 +33:06:45.4: 13.01 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:41.55 +33:06:45.4: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 1902080662798445696,2461179.7895,9.35,0.05,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
Gaia DR3 1902080662798445696 20260519.2895 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 19.2895 2461179.7895 9.42 22:22:56.89 +33:12:02.1
90.39475 -20.12718 galactic Peg Second-epoch detections are separated by 1.9" and 1.6 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 1902137837403010432 | 22:22:56.72 +33:12:05.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:56.89 +33:12:02.1: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:56.89 +33:12:02.1: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 1902137837403010432,2461179.7895,9.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902137837403010432 20260519.2895 9.42CV 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 19.2895 2461179.7895 9.45 22:23:38.23 +33:32:00.0
90.72259 -19.93599 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902152990046950784 | 22:23:38.20 +33:32:01.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.635+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:38.23 +33:32:00.0: 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 22:23:38.23 +33:32:00.0: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 1902152990046950784,2461179.7895,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902152990046950784 20260519.2895 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.44 22:17:38.58 +32:56:02.4
89.26729 -19.69972 galactic Peg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1899035015590241408 | 22:17:38.65 +32:56:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.616+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:38.58 +32:56:02.4: 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 22:17:38.58 +32:56:02.4: 12.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 1899035015590241408,2461179.7895,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899035015590241408 20260519.2895 9.44CV 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 19.2895 2461179.7895 9.42 22:21:33.47 +32:52:45.0
89.94394 -20.22285 galactic Peg Second-epoch detections are separated by 0.7" and 1.5 pix
The object was found in VSX19" CSS_J222132.2+325234
Type: EW
# Max. Min./Amp. JD0 Period
14.110 CV Y 0.260 CV 0.319420000000
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 22:21:33.47 +32:52:45.0: 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 22:21:33.47 +32:52:45.0: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 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
CSS_J222132.2+325234,2461179.7895,9.42,0.05,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
CSS_J222132.2+325234 20260519.2895 9.42CV 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 19.2895 2461179.7895 9.47 22:24:05.46 +33:35:00.5
90.83565 -19.94848 galactic Peg Second-epoch detections are separated by 1.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902174086926456192 | 22:24:05.49 +33:35:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:05.46 +33:35:00.5: 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 22:24:05.46 +33:35:00.5: 12.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 1902174086926456192,2461179.7895,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902174086926456192 20260519.2895 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.48 22:20:23.55 +33:06:53.7
89.87686 -19.88922 galactic Peg Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902054343238512384 | 22:20:23.69 +33:06:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.635+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:23.55 +33:06:53.7: 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 22:20:23.55 +33:06:53.7: 12.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 1902054343238512384,2461179.7895,9.48,0.05,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
Gaia DR3 1902054343238512384 20260519.2895 9.48CV 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 19.2895 2461179.7895 9.56 22:24:20.52 +34:10:17.0
91.23502 -19.49347 galactic Peg Second-epoch detections are separated by 1.1" and 1.6 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 J336.0817+34.1648 | 22:24:20.58 +34:09:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.917+/-0.024 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:20.52 +34:10:17.0: 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 22:24:20.52 +34:10:17.0: 12.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 J336.0817+34.1648,2461179.7895,9.56,0.05,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
ATO J336.0817+34.1648 20260519.2895 9.56CV 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 19.2895 2461179.7895 9.49 22:24:23.17 +33:12:16.0
90.66047 -20.29547 galactic Peg Second-epoch detections are separated by 0.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902093955718232576 | 22:24:23.08 +33:12:18.5 (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 22:24:23.17 +33:12:16.0: 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 22:24:23.17 +33:12:16.0: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.46 +/- 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 1902093955718232576,2461179.7895,9.49,0.05,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
Gaia DR3 1902093955718232576 20260519.2895 9.49CV 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 19.2895 2461179.7895 9.54 22:20:28.76 +32:59:00.9
89.81165 -20.00679 galactic Peg Second-epoch detections are separated by 0.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902027027246492800 | 22:20:28.91 +32:59:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.666+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:28.76 +32:59:00.9: 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 22:20:28.76 +32:59:00.9: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902027027246492800,2461179.7895,9.54,0.05,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
Gaia DR3 1902027027246492800 20260519.2895 9.54CV 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 19.2895 2461179.7895 9.53 22:20:22.40 +32:56:11.9
89.76339 -20.03214 galactic Peg Second-epoch detections are separated by 1.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902025721576309248 | 22:20:22.55 +32:56:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.683+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:22.40 +32:56:11.9: 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 22:20:22.40 +32:56:11.9: 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 1902025721576309248,2461179.7895,9.53,0.05,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
Gaia DR3 1902025721576309248 20260519.2895 9.53CV 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 19.2895 2461179.7895 9.52 22:23:07.16 +33:08:02.2
90.38545 -20.20233 galactic Peg Second-epoch detections are separated by 0.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902090313585969664 | 22:23:07.00 +33:08:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 22:23:07.16 +33:08:02.2: 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 22:23:07.16 +33:08:02.2: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 1902090313585969664,2461179.7895,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902090313585969664 20260519.2895 9.52CV 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 19.2895 2461179.7895 9.59 22:23:55.36 +34:07:37.3
91.13251 -19.48096 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905208051825012096 | 22:23:55.40 +34:07:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.683+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:55.36 +34:07:37.3: 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 22:23:55.36 +34:07:37.3: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1905208051825012096,2461179.7895,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905208051825012096 20260519.2895 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.63 22:22:50.68 +33:02:29.3
90.27878 -20.24524 galactic Peg Second-epoch detections are separated by 0.8" and 1.6 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 1901995725525177216 | 22:22:50.56 +33:02:32.0 (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 22:22:50.68 +33:02:29.3: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:50.68 +33:02:29.3: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901995725525177216,2461179.7895,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901995725525177216 20260519.2895 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.64 22:19:46.52 +33:02:15.5
89.71721 -19.87708 galactic Peg Second-epoch detections are separated by 1.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.9443+33.0379 | 22:19:46.64 +33:02:16.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.520+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:46.52 +33:02:15.5: 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 22:19:46.52 +33:02:15.5: 12.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.9443+33.0379,2461179.7895,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.9443+33.0379 20260519.2895 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.23 21:42:50.22 +37:29:33.0
86.48854 -11.69469 galactic Cyg Second-epoch detections are separated by 0.9" and 1.6 pix
The object was found in VSX 1" Gaia DR3 1952708225458525824
Type: ROT
# Max. Min./Amp. JD0 Period
12.530 G 12.570 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 21:42:50.22 +37:29:33.0: 12.62 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:50.22 +37:29:33.0: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952708225458525824,2461179.7895,10.23,0.05,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 1952708225458525824 20260519.2895 10.23CV 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 19.2895 2461179.7895 9.62 22:20:23.52 +32:54:15.2
89.74677 -20.06081 galactic Peg Second-epoch detections are separated by 0.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902024175388086400 | 22:20:23.68 +32:54:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.676+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:23.52 +32:54:15.2: 10.07 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:23.52 +32:54:15.2: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902024175388086400,2461179.7895,9.62,0.05,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
Gaia DR3 1902024175388086400 20260519.2895 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 19.2895 2461179.7895 9.62 22:24:35.31 +33:46:20.4
91.04016 -19.85151 galactic Peg Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902180065521047552 | 22:24:35.47 +33:46:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.506+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:35.31 +33:46:20.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:35.31 +33:46:20.4: 12.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 1902180065521047552,2461179.7895,9.62,0.05,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
Gaia DR3 1902180065521047552 20260519.2895 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 19.2895 2461179.7895 9.68 22:19:48.19 +33:01:21.3
89.71295 -19.89272 galactic Peg Second-epoch detections are separated by 1.3" and 1.6 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 1902029638586465792 | 22:19:48.27 +33:01:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.655+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:48.19 +33:01:21.3: 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 22:19:48.19 +33:01:21.3: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 1902029638586465792,2461179.7895,9.68,0.05,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
Gaia DR3 1902029638586465792 20260519.2895 9.68CV 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 19.2895 2461179.7895 9.74 22:19:14.40 +32:50:53.6
89.50274 -19.96560 galactic Peg Second-epoch detections are separated by 0.5" and 1.6 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 J334.8106+32.8483 | 22:19:14.55 +32:50:54.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.612+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:14.40 +32:50:53.6: 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 22:19:14.40 +32:50:53.6: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.8106+32.8483,2461179.7895,9.74,0.05,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
ATO J334.8106+32.8483 20260519.2895 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 19.2895 2461179.7895 9.69 22:18:08.29 +32:50:45.1
89.30170 -19.83210 galactic Peg Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1899021752731311616 | 22:18:08.34 +32:50:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.029 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:08.29 +32:50:45.1: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:08.29 +32:50:45.1: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 1899021752731311616,2461179.7895,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899021752731311616 20260519.2895 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.12 21:27:28.55 +35:23:04.1
82.72062 -11.10935 galactic Cyg Second-epoch detections are separated by 2.0" and 1.3 pix
The object was found in VSX13" Gaia DR3 1951314727610397696
Type: E
# Max. Min./Amp. JD0 Period
18.840 G 19.590 G 0.297879000000
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 21:27:28.55 +35:23:04.1: 10.96 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:28.55 +35:23:04.1: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951314727610397696,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951314727610397696 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.82 22:16:43.90 +33:05:24.7
89.20102 -19.46097 galactic Peg Second-epoch detections are separated by 0.5" and 1.5 pix
The object was found in VSX20" Gaia DR3 1899086967514616832
Type: ROT
# Max. Min./Amp. JD0 Period
16.810 G 16.830 G 0.464305000000 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 22:16:43.90 +33:05:24.7: 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 22:16:43.90 +33:05:24.7: 12.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 1899086967514616832,2461179.7895,9.82,0.05,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
Gaia DR3 1899086967514616832 20260519.2895 9.82CV 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 19.2895 2461179.7895 9.71 22:23:44.34 +32:54:13.3
90.35889 -20.46552 galactic Peg Second-epoch detections are separated by 0.6" and 1.6 pix
The object was found in VSX 2" ZTF J222344.31+325415.0
Type: SR
# Max. Min./Amp. JD0 Period
12.655 g Y 0.093 g 2458656.47660 63.170119700000
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 22:23:44.34 +32:54:13.3: 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 22:23:44.34 +32:54:13.3: 12.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J222344.31+325415.0,2461179.7895,9.71,0.05,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
ZTF J222344.31+325415.0 20260519.2895 9.71CV 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 19.2895 2461179.7895 9.74 22:20:57.87 +32:46:23.1
89.77019 -20.23738 galactic Peg Second-epoch detections are separated by 1.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902008954024017536 | 22:20:57.97 +32:46:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.679+/-0.023 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:57.87 +32:46:23.1: 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 22:20:57.87 +32:46:23.1: 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
Gaia DR3 1902008954024017536,2461179.7895,9.74,0.05,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 1902008954024017536 20260519.2895 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 19.2895 2461179.7895 10.33 21:21:47.69 +35:29:50.1
81.97388 -10.20767 galactic Cyg Second-epoch detections are separated by 1.2" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 21:21:47.69 +35:29:50.1: 11.09 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:47.69 +35:29:50.1: 12.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855474216027817600,2461179.7895,10.33,0.05,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
Gaia DR3 1855474216027817600 20260519.2895 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 19.2895 2461179.7895 10.45 21:10:27.84 +36:47:46.3
81.34070 -7.65277 galactic Cyg Second-epoch detections are separated by 0.8" and 1.6 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 | 21:10:27.84 +36:47:46.3 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:27.84 +36:47:46.3: 11.87 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:27.84 +36:47:46.3: 12.63 +/- 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
target,2461179.7895,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.81 22:18:25.16 +32:55:08.1
89.39805 -19.80752 galactic Peg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was found in VSX 2" ASASSN-V J221825.28+325509.9
Type: EA
# Max. Min./Amp. JD0 Period
12.000 V 12.410 V 2457595.91900 1.719130000000
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 22:18:25.16 +32:55:08.1: 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 22:18:25.16 +32:55:08.1: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J221825.28+325509.9,2461179.7895,9.81,0.05,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
ASASSN-V J221825.28+325509.9 20260519.2895 9.81CV 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 19.2895 2461179.7895 10.26 21:24:58.58 +36:59:14.2
83.50818 -9.61832 galactic Cyg Second-epoch detections are separated by 1.0" and 1.6 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 1963742614913936384 | 21:24:56.32 +36:59:31.0 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.690+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:58.58 +36:59:14.2: 11.09 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:58.58 +36:59:14.2: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963742614913936384,2461179.7895,10.26,0.05,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 1963742614913936384 20260519.2895 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 19.2895 2461179.7895 9.80 22:20:34.59 +33:02:40.5
89.86693 -19.96888 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902027473923119744 | 22:20:34.71 +33:02:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.358+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:34.59 +33:02:40.5: 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 22:20:34.59 +33:02:40.5: 12.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 1902027473923119744,2461179.7895,9.80,0.05,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 1902027473923119744 20260519.2895 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 19.2895 2461179.7895 9.84 22:18:20.23 +32:53:58.5
89.37116 -19.81308 galactic Peg Second-epoch detections are separated by 1.2" and 1.5 pix
The object was found in VSX 2" Gaia DR3 1899022302487122176
Type: ROT
# Max. Min./Amp. JD0 Period
11.890 G 11.930 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 22:18:20.23 +32:53:58.5: 12.80 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:20.23 +32:53:58.5: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 1899022302487122176,2461179.7895,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899022302487122176 20260519.2895 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.84 22:22:33.42 +33:34:54.5
90.55551 -19.76779 galactic Peg Second-epoch detections are separated by 1.4" and 1.4 pix
The object was found in VSX 2" Gaia DR3 1902159445379530880
Type: ROT
# Max. Min./Amp. JD0 Period
11.850 G 11.890 G 10.106000000000 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 22:22:33.42 +33:34:54.5: 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 22:22:33.42 +33:34:54.5: 12.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 1902159445379530880,2461179.7895,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902159445379530880 20260519.2895 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.81 22:24:14.74 +33:37:32.5
90.88935 -19.93198 galactic Peg Second-epoch detections are separated by 1.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902174258725145216 | 22:24:14.78 +33:37:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.759+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:14.74 +33:37:32.5: 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 22:24:14.74 +33:37:32.5: 12.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 1902174258725145216,2461179.7895,9.81,0.05,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
Gaia DR3 1902174258725145216 20260519.2895 9.81CV 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 19.2895 2461179.7895 9.81 22:20:37.31 +33:23:33.2
90.08921 -19.69057 galactic Peg Second-epoch detections are separated by 0.5" and 1.7 pix
The object was found in VSX 2" ASASSN-V J222037.45+332333.8
Type: SR
# Max. Min./Amp. JD0 Period
12.180 V 12.310 V 2457927.01000 41.670000000000
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 22:20:37.31 +33:23:33.2: 12.05 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:37.31 +33:23:33.2: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J222037.45+332333.8,2461179.7895,9.81,0.05,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
ASASSN-V J222037.45+332333.8 20260519.2895 9.81CV 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 19.2895 2461179.7895 9.96 22:19:23.14 +32:59:21.0
89.61658 -19.86894 galactic Peg Second-epoch detections are separated by 0.2" and 1.6 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 J334.8419+32.9908 | 22:19:23.22 +32:59:20.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.684+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:23.14 +32:59:21.0: 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 22:19:23.14 +32:59:21.0: 12.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 J334.8419+32.9908,2461179.7895,9.96,0.05,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
ATO J334.8419+32.9908 20260519.2895 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 19.2895 2461179.7895 9.84 22:24:27.88 +33:37:47.6
90.93183 -19.95436 galactic Peg Second-epoch detections are separated by 0.7" and 1.6 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 1902174499243315840 | 22:24:27.94 +33:37:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.668+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:27.88 +33:37:47.6: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:27.88 +33:37:47.6: 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
Gaia DR3 1902174499243315840,2461179.7895,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902174499243315840 20260519.2895 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.95 22:20:39.20 +32:54:15.2
89.79435 -20.09262 galactic Peg Second-epoch detections are separated by 0.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902013764387366016 | 22:20:39.33 +32:54:16.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.249+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:39.20 +32:54:15.2: 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 22:20:39.20 +32:54:15.2: 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 1902013764387366016,2461179.7895,9.95,0.05,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 1902013764387366016 20260519.2895 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 19.2895 2461179.7895 10.01 22:20:39.00 +32:50:13.8
89.75235 -20.14686 galactic Peg Second-epoch detections are separated by 1.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.1630+32.8376 | 22:20:39.14 +32:50:15.4 (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 22:20:39.00 +32:50:13.8: 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 22:20:39.00 +32:50:13.8: 13.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 J335.1630+32.8376,2461179.7895,10.01,0.05,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
ATO J335.1630+32.8376 20260519.2895 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.87 22:23:07.90 +33:23:02.6
90.53988 -19.99854 galactic Peg Second-epoch detections are separated by 2.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902144674990141056 | 22:23:07.95 +33:23:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:07.90 +33:23:02.6: 12.70 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:07.90 +33:23:02.6: 12.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 1902144674990141056,2461179.7895,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902144674990141056 20260519.2895 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.38 21:50:26.30 +41:51:43.1
90.51857 -9.34288 galactic Cyg Second-epoch detections are separated by 0.5" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:26.30 +41:51:43.1 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:26.30 +41:51:43.1: 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 21:50:26.30 +41:51:43.1: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461179.7895,10.38,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.53 21:17:37.39 +36:35:15.8
82.17675 -8.84379 galactic Cyg Second-epoch detections are separated by 0.9" and 1.6 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 | 21:17:37.39 +36:35:15.8 (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 21:17:37.39 +36:35:15.8: 11.64 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:37.39 +36:35:15.8: 12.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 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,2461179.7895,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.97 22:23:02.72 +32:42:37.5
90.11322 -20.54069 galactic Peg Second-epoch detections are separated by 0.9" and 1.6 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 J335.7572+32.7112 | 22:23:02.92 +32:42:36.0 (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 22:23:02.72 +32:42:37.5: 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 22:23:02.72 +32:42:37.5: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J335.7572+32.7112,2461179.7895,9.97,0.05,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 J335.7572+32.7112 20260519.2895 9.97CV 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 19.2895 2461179.7895 9.90 22:23:31.33 +32:43:59.5
90.21496 -20.57943 galactic Peg Second-epoch detections are separated by 2.2" and 1.8 pix
The object was found in VSX 5" ASASSN-V J222331.65+324356.9
Type: SR
# Max. Min./Amp. JD0 Period
12.440 V 12.530 V 2456892.00000 135.000000000000
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 22:23:31.33 +32:43:59.5: 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 22:23:31.33 +32:43:59.5: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J222331.65+324356.9,2461179.7895,9.90,0.05,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
ASASSN-V J222331.65+324356.9 20260519.2895 9.90CV 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 19.2895 2461179.7895 10.36 21:29:32.56 +33:47:11.0
81.87985 -12.54380 galactic Cyg Second-epoch detections are separated by 1.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:32.56 +33:47:11.0 (user input) | T | P | (position from user input) J-Ks=0.934+/-0.024 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:32.56 +33:47:11.0: 10.82 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:32.56 +33:47:11.0: 12.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461179.7895,10.36,0.05,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
target 20260519.2895 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.04 22:18:36.65 +32:58:58.0
89.47240 -19.77925 galactic Peg Second-epoch detections are separated by 0.5" and 1.6 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 1905027796338994432 | 22:18:36.73 +32:58:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.041 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:36.65 +32:58:58.0: 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 22:18:36.65 +32:58:58.0: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 1905027796338994432,2461179.7895,10.04,0.05,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
Gaia DR3 1905027796338994432 20260519.2895 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 19.2895 2461179.7895 9.99 22:20:45.94 +32:42:31.8
89.69419 -20.26552 galactic Peg Second-epoch detections are separated by 1.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902006892439722496 | 22:20:46.05 +32:42:32.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.471+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:45.94 +32:42:31.8: 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 22:20:45.94 +32:42:31.8: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 1902006892439722496,2461179.7895,9.99,0.05,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
Gaia DR3 1902006892439722496 20260519.2895 9.99CV 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 19.2895 2461179.7895 10.04 22:19:44.77 +33:18:41.9
89.88115 -19.65056 galactic Peg Second-epoch detections are separated by 1.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905062710131608832 | 22:19:44.89 +33:18:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.313+/-0.032 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:44.77 +33:18:41.9: 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 22:19:44.77 +33:18:41.9: 13.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 1905062710131608832,2461179.7895,10.04,0.05,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
Gaia DR3 1905062710131608832 20260519.2895 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 19.2895 2461179.7895 9.98 22:20:50.94 +32:53:15.3
89.81974 -20.12997 galactic Peg Second-epoch detections are separated by 0.5" and 1.6 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 1902013450851782528 | 22:20:51.10 +32:53:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.690+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:50.94 +32:53:15.3: 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 22:20:50.94 +32:53:15.3: 12.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 1902013450851782528,2461179.7895,9.98,0.05,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
Gaia DR3 1902013450851782528 20260519.2895 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.08 22:21:35.05 +32:41:15.4
89.83086 -20.38247 galactic Peg Second-epoch detections are separated by 1.6" and 1.6 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 1901959849659956864 | 22:21:35.02 +32:41:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.660+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:35.05 +32:41:15.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:35.05 +32:41:15.4: 13.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 1901959849659956864,2461179.7895,10.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901959849659956864 20260519.2895 10.08CV 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 19.2895 2461179.7895 10.49 21:22:36.14 +35:35:48.6
82.16287 -10.25566 galactic Cyg Second-epoch detections are separated by 1.1" and 1.6 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 1855481710751928960 | 21:22:38.77 +35:35:48.8 (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 21:22:36.14 +35:35:48.6: 10.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:36.14 +35:35:48.6: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855481710751928960,2461179.7895,10.49,0.05,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
Gaia DR3 1855481710751928960 20260519.2895 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 19.2895 2461179.7895 10.12 22:24:31.23 +34:22:25.5
91.38845 -19.34728 galactic Peg Second-epoch detections are separated by 2.5" and 1.2 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 1905588895164731264 | 22:24:31.31 +34:22:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.719+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:31.23 +34:22:25.5: 12.07 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:31.23 +34:22:25.5: 13.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 1905588895164731264,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905588895164731264 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.12 22:21:46.71 +33:32:37.6
90.39116 -19.70599 galactic Peg Second-epoch detections are separated by 0.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902161506965572224 | 22:21:46.77 +33:32:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.624+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:46.71 +33:32:37.6: 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 22:21:46.71 +33:32:37.6: 13.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 1902161506965572224,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902161506965572224 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.06 22:22:57.67 +33:36:03.3
90.64052 -19.80020 galactic Peg Second-epoch detections are separated by 3.5" and 1.2 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 1902165187753918080 | 22:22:57.63 +33:36:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.279+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:57.67 +33:36:03.3: 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 22:22:57.67 +33:36:03.3: 13.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 1902165187753918080,2461179.7895,10.06,0.05,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
Gaia DR3 1902165187753918080 20260519.2895 10.06CV 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 19.2895 2461179.7895 10.26 22:11:47.62 +38:26:20.1
91.65350 -14.55032 galactic Lac Second-epoch detections are separated by 1.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955443634287437568 | 22:11:47.78 +38:26:21.9 (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 22:11:47.62 +38:26:20.1: 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 22:11:47.62 +38:26:20.1: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 1955443634287437568,2461179.7895,10.26,0.05,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 1955443634287437568 20260519.2895 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 19.2895 2461179.7895 10.23 22:02:42.94 +33:22:25.8
86.93064 -17.45279 galactic Peg Second-epoch detections are separated by 2.1" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:42.94 +33:22:25.8 (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 22:02:42.94 +33:22:25.8: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.94 +33:22:25.8: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461179.7895,10.23,0.05,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 20260519.2895 10.23CV 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 19.2895 2461179.7895 10.08 22:22:28.49 +33:46:01.3
90.65311 -19.60607 galactic Peg Second-epoch detections are separated by 1.4" and 1.4 pix
The object was found in VSX 1" Gaia DR3 1905172828794747264
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.170 G 12.200 G 0.044983700000 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 22:22:28.49 +33:46:01.3: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:28.49 +33:46:01.3: 13.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.14 +/- 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 1905172828794747264,2461179.7895,10.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905172828794747264 20260519.2895 10.08CV 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 19.2895 2461179.7895 10.12 22:23:45.42 +33:03:10.9
90.45309 -20.34502 galactic Peg Second-epoch detections are separated by 2.1" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902085571942079104 | 22:23:45.39 +33:03:13.3 (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 22:23:45.42 +33:03:10.9: 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 22:23:45.42 +33:03:10.9: 13.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 1902085571942079104,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902085571942079104 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.12 22:23:27.37 +33:57:49.6
90.94981 -19.56054 galactic Peg Second-epoch detections are separated by 1.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902198310541955328 | 22:23:27.38 +33:57:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.326+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:27.37 +33:57:49.6: 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 22:23:27.37 +33:57:49.6: 13.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 1902198310541955328,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902198310541955328 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.17 22:23:36.58 +33:39:32.2
90.79357 -19.82944 galactic Peg Second-epoch detections are separated by 1.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:36.58 +33:39:32.2 (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 22:23:36.58 +33:39:32.2: 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 22:23:36.58 +33:39:32.2: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.14 +/- 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,2461179.7895,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.04 22:24:19.63 +33:45:17.7
90.98208 -19.83513 galactic Peg Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902179790643009408 | 22:24:19.77 +33:45:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.625+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:19.63 +33:45:17.7: 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 22:24:19.63 +33:45:17.7: 13.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 1902179790643009408,2461179.7895,10.04,0.05,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
Gaia DR3 1902179790643009408 20260519.2895 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 19.2895 2461179.7895 10.14 22:21:09.22 +33:14:22.0
90.09162 -19.87974 galactic Peg Second-epoch detections are separated by 0.3" and 1.6 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 1902056885859306752 | 22:21:09.32 +33:14:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.826+/-0.028 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:09.22 +33:14:22.0: 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 22:21:09.22 +33:14:22.0: 13.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 1902056885859306752,2461179.7895,10.14,0.05,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 1902056885859306752 20260519.2895 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 19.2895 2461179.7895 10.24 22:22:51.88 +33:51:23.0
90.77784 -19.57895 galactic Peg Second-epoch detections are separated by 0.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905175066475956352 | 22:22:51.92 +33:51:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.290+/-0.029 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:51.88 +33:51:23.0: 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 22:22:51.88 +33:51:23.0: 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
Gaia DR3 1905175066475956352,2461179.7895,10.24,0.05,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 1905175066475956352 20260519.2895 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.12 22:18:05.10 +32:44:50.7
89.23064 -19.90525 galactic Peg Second-epoch detections are separated by 2.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1899016766270207872 | 22:18:05.20 +32:44:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=0.873+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:05.10 +32:44:50.7: 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 22:18:05.10 +32:44:50.7: 13.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 1899016766270207872,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899016766270207872 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.49 21:42:45.65 +36:52:50.7
86.05998 -12.14038 galactic Cyg Second-epoch detections are separated by 2.8" and 1.9 pix
The object was found in VSX17" Gaia DR3 1952608513496231040
Type: RS
# Max. Min./Amp. JD0 Period
15.130 G 15.270 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 21:42:45.65 +36:52:50.7: 13.22 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:45.65 +36:52:50.7: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952608513496231040,2461179.7895,10.49,0.05,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
Gaia DR3 1952608513496231040 20260519.2895 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 19.2895 2461179.7895 10.05 22:23:15.04 +34:07:35.0
91.01070 -19.40256 galactic Peg Second-epoch detections are separated by 1.6" and 1.6 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 1905205852801653760 | 22:23:15.06 +34:07:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.634+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:15.04 +34:07:35.0: 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 22:23:15.04 +34:07:35.0: 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
Gaia DR3 1905205852801653760,2461179.7895,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905205852801653760 20260519.2895 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.23 22:19:32.53 +33:07:17.7
89.72689 -19.78039 galactic Peg Second-epoch detections are separated by 2.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:32.53 +33:07:17.7 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.536+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:32.53 +33:07:17.7: 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 22:19:32.53 +33:07:17.7: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 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,2461179.7895,10.23,0.05,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 20260519.2895 10.23CV 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 19.2895 2461179.7895 10.20 22:23:10.00 +34:09:20.1
91.01314 -19.36866 galactic Peg Second-epoch detections are separated by 3.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905206162039292928 | 22:23:10.04 +34:09:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.638+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:10.00 +34:09:20.1: 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 22:23:10.00 +34:09:20.1: 13.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 1905206162039292928,2461179.7895,10.20,0.05,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
Gaia DR3 1905206162039292928 20260519.2895 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.19 22:21:07.21 +33:09:50.1
90.03916 -19.93737 galactic Peg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902053106288094080 | 22:21:07.18 +33:09:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.390+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:07.21 +33:09:50.1: 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 22:21:07.21 +33:09:50.1: 13.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 1902053106288094080,2461179.7895,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902053106288094080 20260519.2895 10.19CV 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 19.2895 2461179.7895 10.23 22:24:03.21 +33:02:09.1
90.49712 -20.39453 galactic Peg Second-epoch detections are separated by 0.7" and 1.6 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 1902073653410984192 | 22:24:03.18 +33:02:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.853+/-0.025 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:03.21 +33:02:09.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:03.21 +33:02:09.1: 13.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 1902073653410984192,2461179.7895,10.23,0.05,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 1902073653410984192 20260519.2895 10.23CV 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 19.2895 2461179.7895 10.62 21:26:25.10 +35:51:26.3
82.90521 -10.62263 galactic Cyg Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.6060+35.8609 | 21:26:25.10 +35:51:26.3 (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 21:26:25.10 +35:51:26.3: 11.32 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:25.10 +35:51:26.3: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.34 +/- 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+35.8609,2461179.7895,10.62,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.25 22:21:41.85 +33:15:31.7
90.20231 -19.92944 galactic Peg Second-epoch detections are separated by 2.2" and 1.6 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 1902059389821990784 | 22:21:41.75 +33:15:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:41.85 +33:15:31.7: 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 22:21:41.85 +33:15:31.7: 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 1902059389821990784,2461179.7895,10.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902059389821990784 20260519.2895 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.68 21:26:53.13 +37:31:51.0
84.17001 -9.50075 galactic Cyg Second-epoch detections are separated by 1.4" and 1.6 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 J321.7099+37.5254 | 21:26:53.13 +37:31:51.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.322+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:53.13 +37:31:51.0: 11.91 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:53.13 +37:31:51.0: 12.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.7099+37.5254,2461179.7895,10.68,0.05,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 J321.7099+37.5254 20260519.2895 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 19.2895 2461179.7895 10.15 22:23:43.81 +33:04:00.7
90.45657 -20.33045 galactic Peg Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902085644959668096 | 22:23:43.64 +33:04:02.8 (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 22:23:43.81 +33:04:00.7: 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 22:23:43.81 +33:04:00.7: 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
Gaia DR3 1902085644959668096,2461179.7895,10.15,0.05,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
Gaia DR3 1902085644959668096 20260519.2895 10.15CV 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 19.2895 2461179.7895 10.34 22:22:08.94 +33:00:18.6
90.12931 -20.19129 galactic Peg Second-epoch detections are separated by 2.1" and 1.5 pix
The object was found in VSX 3" Gaia DR3 1902041046019959936
Type: ROT
# Max. Min./Amp. JD0 Period
12.380 G 12.430 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 22:22:08.94 +33:00:18.6: 12.77 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:08.94 +33:00:18.6: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 1902041046019959936,2461179.7895,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902041046019959936 20260519.2895 10.34CV 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 19.2895 2461179.7895 10.24 22:24:06.40 +33:47:07.0
90.96024 -19.78414 galactic Peg Second-epoch detections are separated by 1.6" and 1.6 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 1902180782777121024 | 22:24:06.49 +33:47:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:06.40 +33:47:07.0: 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 22:24:06.40 +33:47:07.0: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 1902180782777121024,2461179.7895,10.24,0.05,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 1902180782777121024 20260519.2895 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.12 22:23:20.66 +32:59:09.3
90.33647 -20.35074 galactic Peg Second-epoch detections are separated by 1.4" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901991842874753408 | 22:23:20.56 +32:59:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:20.66 +32:59:09.3: 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 22:23:20.66 +32:59:09.3: 13.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 1901991842874753408,2461179.7895,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901991842874753408 20260519.2895 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.24 22:22:55.78 +33:33:57.5
90.61358 -19.82515 galactic Peg Second-epoch detections are separated by 1.3" and 1.6 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 1902164328760462592 | 22:22:55.74 +33:33:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.585+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:55.78 +33:33:57.5: 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 22:22:55.78 +33:33:57.5: 13.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 1902164328760462592,2461179.7895,10.24,0.05,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 1902164328760462592 20260519.2895 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.72 21:23:35.23 +38:21:42.0
84.29709 -8.45321 galactic Cyg Second-epoch detections are separated by 1.8" and 1.6 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 J320.8920+38.3544 | 21:23:35.23 +38:21:42.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.383+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:35.23 +38:21:42.0: 10.98 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:35.23 +38:21:42.0: 12.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.8920+38.3544,2461179.7895,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.8920+38.3544 20260519.2895 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.23 22:19:34.44 +33:14:38.1
89.80825 -19.68476 galactic Peg Second-epoch detections are separated by 1.2" and 1.6 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 1905038894534477568 | 22:19:34.55 +33:14:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:34.44 +33:14:38.1: 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 22:19:34.44 +33:14:38.1: 13.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 1905038894534477568,2461179.7895,10.23,0.05,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 1905038894534477568 20260519.2895 10.23CV 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 19.2895 2461179.7895 10.29 22:20:56.39 +32:59:39.1
89.90199 -20.05405 galactic Peg Second-epoch detections are separated by 2.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902037850564117760 | 22:20:56.53 +32:59:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.023 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:56.39 +32:59:39.1: 12.22 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:56.39 +32:59:39.1: 13.49 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 1902037850564117760,2461179.7895,10.29,0.05,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 1902037850564117760 20260519.2895 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 19.2895 2461179.7895 10.34 22:21:03.77 +33:12:54.3
90.06017 -19.88867 galactic Peg Second-epoch detections are separated by 1.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902056744122138112 | 22:21:03.91 +33:12:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:03.77 +33:12:54.3: 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 22:21:03.77 +33:12:54.3: 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
Gaia DR3 1902056744122138112,2461179.7895,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902056744122138112 20260519.2895 10.34CV 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 19.2895 2461179.7895 10.20 22:22:19.37 +32:54:25.7
90.10106 -20.29246 galactic Peg Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.5760+32.9088 | 22:22:19.27 +32:54:27.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:19.37 +32:54:25.7: 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 22:22:19.37 +32:54:25.7: 13.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 J335.5760+32.9088,2461179.7895,10.20,0.05,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
ATO J335.5760+32.9088 20260519.2895 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.29 22:25:19.00 +34:03:17.2
91.34205 -19.70354 galactic Peg Second-epoch detections are separated by 0.4" and 1.4 pix
The object was found in VSX14" Gaia DR3 1902565444346216832
Type: ROT
# Max. Min./Amp. JD0 Period
16.770 G 16.830 G 5.572900000000 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 22:25:19.00 +34:03:17.2: 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 22:25:19.00 +34:03:17.2: 13.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 1902565444346216832,2461179.7895,10.29,0.05,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 1902565444346216832 20260519.2895 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 19.2895 2461179.7895 10.32 22:23:25.02 +33:24:37.2
90.60789 -20.01094 galactic Peg Second-epoch detections are separated by 0.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902147698647118336 | 22:23:24.99 +33:24:39.7 (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 22:23:25.02 +33:24:37.2: 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 22:23:25.02 +33:24:37.2: 13.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 1902147698647118336,2461179.7895,10.32,0.05,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
Gaia DR3 1902147698647118336 20260519.2895 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 19.2895 2461179.7895 10.25 22:21:45.89 +33:23:34.6
90.29659 -19.82779 galactic Peg Second-epoch detections are separated by 1.2" and 1.6 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 1902065540215156096 | 22:21:45.91 +33:23:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:45.89 +33:23:34.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:45.89 +33:23:34.6: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 1902065540215156096,2461179.7895,10.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902065540215156096 20260519.2895 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.34 22:19:23.99 +32:46:40.9
89.48818 -20.04220 galactic Peg Second-epoch detections are separated by 1.8" and 1.6 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 1902016508868500736 | 22:19:24.13 +32:46:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.821+/-0.024 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:23.99 +32:46:40.9: 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 22:19:23.99 +32:46:40.9: 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
Gaia DR3 1902016508868500736,2461179.7895,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902016508868500736 20260519.2895 10.34CV 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 19.2895 2461179.7895 10.22 22:22:58.32 +32:58:41.8
90.26352 -20.31233 galactic Peg Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901994591653819264 | 22:22:58.20 +32:58:44.7 (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 22:22:58.32 +32:58:41.8: 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 22:22:58.32 +32:58:41.8: 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
Gaia DR3 1901994591653819264,2461179.7895,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901994591653819264 20260519.2895 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.29 22:24:08.92 +33:57:54.4
91.07612 -19.64091 galactic Peg Second-epoch detections are separated by 2.3" and 1.2 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 1902200505266931072 | 22:24:09.03 +33:57:56.2 (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 22:24:08.92 +33:57:54.4: 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 22:24:08.92 +33:57:54.4: 13.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 1902200505266931072,2461179.7895,10.29,0.05,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 1902200505266931072 20260519.2895 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 19.2895 2461179.7895 10.26 22:18:37.77 +32:48:16.6
89.36492 -19.92602 galactic Peg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was found in VSX 2" Gaia DR3 1899017870080883584
Type: ROT
# Max. Min./Amp. JD0 Period
12.300 G 12.320 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 22:18:37.77 +32:48:16.6: 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 22:18:37.77 +32:48:16.6: 13.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 1899017870080883584,2461179.7895,10.26,0.05,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 1899017870080883584 20260519.2895 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 19.2895 2461179.7895 10.98 21:13:10.67 +42:30:08.0
85.89918 -4.14883 galactic Cyg Second-epoch detections are separated by 3.9" and 1.9 pix
The object was found in VSX16" Gaia DR3 1969801439378203648
Type: E
# Max. Min./Amp. JD0 Period
18.630 G 19.230 G 1.520640000000
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 21:13:10.67 +42:30:08.0: 11.89 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:10.67 +42:30:08.0: 13.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 1969801439378203648,2461179.7895,10.98,0.05,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
Gaia DR3 1969801439378203648 20260519.2895 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 19.2895 2461179.7895 10.37 22:23:19.94 +33:27:41.0
90.62342 -19.95892 galactic Peg Second-epoch detections are separated by 1.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902150859743177984 | 22:23:22.68 +33:27:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.385+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:19.94 +33:27:41.0: 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 22:23:19.94 +33:27:41.0: 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 1902150859743177984,2461179.7895,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902150859743177984 20260519.2895 10.37CV 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 19.2895 2461179.7895 10.35 22:20:40.74 +33:08:47.3
89.94830 -19.89823 galactic Peg Second-epoch detections are separated by 1.9" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902054618116419456 | 22:20:40.87 +33:08:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.648+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:40.74 +33:08:47.3: 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 22:20:40.74 +33:08:47.3: 13.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 1902054618116419456,2461179.7895,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902054618116419456 20260519.2895 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.34 22:23:01.53 +32:54:18.4
90.22864 -20.37874 galactic Peg Second-epoch detections are separated by 2.6" and 1.8 pix
The object was found in VSX 2" Gaia DR3 1901989678211242240
Type: ROT
# Max. Min./Amp. JD0 Period
12.260 G 12.290 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 22:23:01.53 +32:54:18.4: 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 22:23:01.53 +32:54:18.4: 13.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 1901989678211242240,2461179.7895,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901989678211242240 20260519.2895 10.34CV 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 19.2895 2461179.7895 10.88 21:15:42.98 +33:53:36.6
79.91777 -10.40917 galactic Cyg Second-epoch detections are separated by 2.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.9171+33.8998 | 21:15:42.98 +33:53:36.6 (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 21:15:42.98 +33:53:36.6: 12.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:42.98 +33:53:36.6: 12.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.89 +/- 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+33.8998,2461179.7895,10.88,0.05,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 J318.9171+33.8998 20260519.2895 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 19.2895 2461179.7895 10.22 22:21:49.75 +33:05:15.9
90.12152 -20.08518 galactic Peg Second-epoch detections are separated by 2.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902045444066459008 | 22:21:49.84 +33:05:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:49.75 +33:05:15.9: 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 22:21:49.75 +33:05:15.9: 13.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 1902045444066459008,2461179.7895,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902045444066459008 20260519.2895 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.45 22:20:21.50 +32:42:46.3
89.62231 -20.21252 galactic Peg Second-epoch detections are separated by 2.0" and 1.6 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 | 22:20:21.50 +32:42:46.3 (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 22:20:21.50 +32:42:46.3: 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 22:20:21.50 +32:42:46.3: 13.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461179.7895,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.39 22:22:07.66 +32:48:47.3
90.00765 -20.34578 galactic Peg Second-epoch detections are separated by 1.6" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:07.66 +32:48:47.3 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:07.66 +32:48:47.3: 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 22:22:07.66 +32:48:47.3: 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
target,2461179.7895,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.36 22:19:10.61 +33:01:16.8
89.59870 -19.81728 galactic Peg Second-epoch detections are separated by 1.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905026701125535232 | 22:19:10.70 +33:01:18.5 (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 22:19:10.61 +33:01:16.8: 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 22:19:10.61 +33:01:16.8: 13.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 1905026701125535232,2461179.7895,10.36,0.05,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 1905026701125535232 20260519.2895 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.41 22:14:49.17 +32:48:44.8
88.68378 -19.44679 galactic Peg Second-epoch detections are separated by 1.6" and 1.2 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 J333.7053+32.8169 | 22:14:49.17 +32:48:44.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:14:49.17 +32:48:44.8: 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 22:14:49.17 +32:48:44.8: 13.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 J333.7053+32.8169,2461179.7895,10.41,0.05,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 J333.7053+32.8169 20260519.2895 10.41CV 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 19.2895 2461179.7895 10.79 21:31:02.09 +37:39:41.7
84.85980 -9.98079 galactic Cyg Second-epoch detections are separated by 1.2" and 1.6 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 J322.7506+37.6620 | 21:31:00.15 +37:39:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:02.09 +37:39:41.7: 13.37 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:02.09 +37:39:41.7: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7506+37.6620,2461179.7895,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7506+37.6620 20260519.2895 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.44 22:20:42.31 +33:18:15.6
90.05011 -19.77262 galactic Peg Second-epoch detections are separated by 1.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:20:42.31 +33:18:15.6 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:42.31 +33:18:15.6: 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 22:20:42.31 +33:18:15.6: 13.51 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461179.7895,10.44,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.43 22:23:55.51 +33:00:55.5
90.46111 -20.39601 galactic Peg Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.9704+33.0089 | 22:23:55.51 +33:00:55.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:55.51 +33:00:55.5: 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 22:23:55.51 +33:00:55.5: 13.74 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 J335.9704+33.0089,2461179.7895,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.9704+33.0089 20260519.2895 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.41 22:24:04.60 +34:24:03.0
91.32458 -19.27322 galactic Peg Second-epoch detections are separated by 2.1" and 1.2 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 1905590819310072064 | 22:24:04.71 +34:24:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.658+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:04.60 +34:24:03.0: 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 22:24:04.60 +34:24:03.0: 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
Gaia DR3 1905590819310072064,2461179.7895,10.41,0.05,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 1905590819310072064 20260519.2895 10.41CV 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 19.2895 2461179.7895 10.36 22:19:26.54 +33:03:40.7
89.67153 -19.81723 galactic Peg Second-epoch detections are separated by 1.6" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905032709781577984 | 22:19:26.66 +33:03:41.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:26.54 +33:03:40.7: 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 22:19:26.54 +33:03:40.7: 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
Gaia DR3 1905032709781577984,2461179.7895,10.36,0.05,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 1905032709781577984 20260519.2895 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.40 22:21:16.32 +33:39:10.4
90.36615 -19.55607 galactic Peg Second-epoch detections are separated by 1.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:16.32 +33:39:10.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:16.32 +33:39:10.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:16.32 +33:39:10.4: 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,2461179.7895,10.40,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.54 22:20:55.87 +41:36:26.6
95.00013 -12.95940 galactic Lac Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.2412+41.5961 | 22:20:55.87 +41:36:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.076+/-0.026 (M)
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 +41:36:26.6: 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 22:20:55.87 +41:36:26.6: 13.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.30 +/- 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+41.5961,2461179.7895,10.54,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.46 22:22:17.26 +32:41:43.5
89.96472 -20.46142 galactic Peg Second-epoch detections are separated by 2.5" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:17.26 +32:41:43.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:17.26 +32:41:43.5: 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 22:22:17.26 +32:41:43.5: 13.46 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461179.7895,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.38 22:24:46.42 +33:23:51.6
90.84833 -20.18223 galactic Peg Second-epoch detections are separated by 1.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902097842667042944 | 22:24:46.50 +33:23:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.672+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:46.42 +33:23:51.6: 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 22:24:46.42 +33:23:51.6: 13.51 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 1902097842667042944,2461179.7895,10.38,0.05,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
Gaia DR3 1902097842667042944 20260519.2895 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 19.2895 2461179.7895 10.46 22:21:01.94 +33:19:23.0
90.12090 -19.79682 galactic Peg Second-epoch detections are separated by 1.4" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902064135764090496 | 22:20:59.16 +33:19:09.4 (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 22:21:01.94 +33:19:23.0: 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 22:21:01.94 +33:19:23.0: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902064135764090496,2461179.7895,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902064135764090496 20260519.2895 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.83 21:17:44.52 +33:45:12.7
80.10663 -10.81183 galactic Cyg Second-epoch detections are separated by 2.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:17:44.52 +33:45:12.7 (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 21:17:44.52 +33:45:12.7: 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 21:17:44.52 +33:45:12.7: 13.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.06 +/- 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,2461179.7895,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.49 22:23:48.00 +33:17:20.9
90.60436 -20.15611 galactic Peg Second-epoch detections are separated by 2.1" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:48.00 +33:17:20.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:48.00 +33:17:20.9: 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 22:23:48.00 +33:17:20.9: 13.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461179.7895,10.49,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.47 22:23:48.10 +34:10:12.1
91.13648 -19.43134 galactic Peg Second-epoch detections are separated by 0.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:48.10 +34:10:12.1 (user input) | T | P | (position from user input) 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 22:23:48.10 +34:10:12.1: 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 22:23:48.10 +34:10:12.1: 13.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.37 +/- 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,2461179.7895,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.45 22:20:05.95 +32:43:47.6
89.58559 -20.16698 galactic Peg Second-epoch detections are separated by 3.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902005105733196032 | 22:20:06.10 +32:43:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.413+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:05.95 +32:43:47.6: 11.84 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:05.95 +32:43:47.6: 13.34 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 1902005105733196032,2461179.7895,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902005105733196032 20260519.2895 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.03 21:34:48.86 +41:16:17.5
87.90506 -7.85624 galactic Cyg Second-epoch detections are separated by 1.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.7026+41.2683 | 21:34:48.86 +41:16:17.5 (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 21:34:48.86 +41:16:17.5: 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 21:34:48.86 +41:16:17.5: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 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+41.2683,2461179.7895,11.03,0.05,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 J323.7026+41.2683 20260519.2895 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 19.2895 2461179.7895 10.41 22:23:28.06 +32:56:28.4
90.33187 -20.40220 galactic Peg Second-epoch detections are separated by 1.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.8741+32.9480 | 22:23:28.06 +32:56:28.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:28.06 +32:56:28.4: 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 22:23:28.06 +32:56:28.4: 13.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 J335.8741+32.9480,2461179.7895,10.41,0.05,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 J335.8741+32.9480 20260519.2895 10.41CV 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 19.2895 2461179.7895 10.82 21:40:40.87 +36:19:20.7
85.36012 -12.27467 galactic Cyg Second-epoch detections are separated by 1.0" and 1.6 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 J325.1711+36.3226 | 21:40:38.96 +36:19:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:40.87 +36:19:20.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:40.87 +36:19:20.7: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1711+36.3226,2461179.7895,10.82,0.05,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 J325.1711+36.3226 20260519.2895 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 19.2895 2461179.7895 10.34 22:23:00.98 +33:29:38.4
90.58565 -19.89454 galactic Peg Second-epoch detections are separated by 1.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902146221178352896 | 22:23:00.94 +33:29:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:00.98 +33:29:38.4: 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 22:23:00.98 +33:29:38.4: 13.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 1902146221178352896,2461179.7895,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902146221178352896 20260519.2895 10.34CV 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 19.2895 2461179.7895 10.80 21:41:29.00 +37:46:46.0
86.48045 -11.30214 galactic Cyg Second-epoch detections are separated by 1.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3761+37.7784 | 21:41:29.00 +37:46:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.363+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:29.00 +37:46:46.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:29.00 +37:46:46.0: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 J325.3761+37.7784,2461179.7895,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3761+37.7784 20260519.2895 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.41 22:21:13.43 +32:41:43.0
89.76960 -20.33239 galactic Peg Second-epoch detections are separated by 2.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:13.43 +32:41:43.0 (user input) | T | P | (position from user input) J-Ks=0.738+/-0.023 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:13.43 +32:41:43.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:13.43 +32:41:43.0: 13.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.39 +/- 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,2461179.7895,10.41,0.05,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
target 20260519.2895 10.41CV 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 19.2895 2461179.7895 10.95 21:24:39.30 +36:58:43.5
83.45609 -9.57892 galactic Cyg Second-epoch detections are separated by 6.9" and 0.6 pix
The object was found in VSX24" 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 21:24:39.30 +36:58:43.5: 11.65 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:39.30 +36:58:43.5: 13.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 1963742408760031616,2461179.7895,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963742408760031616 20260519.2895 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 19.2895 2461179.7895 10.43 22:22:40.25 +34:04:04.1
90.87072 -19.38237 galactic Peg Second-epoch detections are separated by 1.8" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1905204645912466304 | 22:22:40.42 +34:04:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:40.25 +34:04:04.1: 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 22:22:40.25 +34:04:04.1: 13.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 1905204645912466304,2461179.7895,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905204645912466304 20260519.2895 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.55 22:20:39.92 +33:27:29.1
90.13729 -19.64234 galactic Peg Second-epoch detections are separated by 1.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.1773+33.4601 | 22:20:42.57 +33:27:36.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.562+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:39.92 +33:27:29.1: 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 22:20:39.92 +33:27:29.1: 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
ATO J335.1773+33.4601,2461179.7895,10.55,0.05,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
ATO J335.1773+33.4601 20260519.2895 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 19.2895 2461179.7895 10.39 22:23:53.79 +32:58:14.7
90.42868 -20.42929 galactic Peg Second-epoch detections are separated by 2.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902072863137008256 | 22:23:53.71 +32:58:17.6 (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 22:23:53.79 +32:58:14.7: 11.78 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:53.79 +32:58:14.7: 13.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 1902072863137008256,2461179.7895,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902072863137008256 20260519.2895 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.85 21:32:54.29 +35:30:10.2
83.61204 -11.79735 galactic Cyg Second-epoch detections are separated by 2.1" and 1.6 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 1951363316579121152 | 21:32:51.70 +35:29:57.4 (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 21:32:54.29 +35:30:10.2: 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 21:32:54.29 +35:30:10.2: 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
Gaia DR3 1951363316579121152,2461179.7895,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951363316579121152 20260519.2895 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.07 21:14:38.33 +37:33:54.1
82.48013 -7.73957 galactic Cyg Second-epoch detections are separated by 2.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1868691174732587776 | 21:14:40.87 +37:33:33.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:38.33 +37:33:54.1: 11.38 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:38.33 +37:33:54.1: 13.34 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 1868691174732587776,2461179.7895,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1868691174732587776 20260519.2895 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.51 22:23:42.36 +33:58:37.1
91.00301 -19.57910 galactic Peg Second-epoch detections are separated by 1.3" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:42.36 +33:58:37.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.378+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:42.36 +33:58:37.1: 13.28 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:42.36 +33:58:37.1: 13.68 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461179.7895,10.51,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.54 22:21:08.21 +33:31:44.5
90.26600 -19.64112 galactic Peg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:08.21 +33:31:44.5 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.024 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:08.21 +33:31:44.5: 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 22:21:08.21 +33:31:44.5: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 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,2461179.7895,10.54,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.68 22:07:05.37 +37:55:15.6
90.56819 -14.41396 galactic Lac Second-epoch detections are separated by 0.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.7704+37.9239 | 22:07:05.37 +37:55:15.6 (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 22:07:05.37 +37:55:15.6: 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 22:07:05.37 +37:55:15.6: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 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+37.9239,2461179.7895,10.68,0.05,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 J331.7704+37.9239 20260519.2895 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 19.2895 2461179.7895 10.37 22:22:44.70 +33:19:20.4
90.43183 -20.00303 galactic Peg Second-epoch detections are separated by 0.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:44.70 +33:19:20.4 (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 22:22:44.70 +33:19:20.4: 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 22:22:44.70 +33:19:20.4: 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
target,2461179.7895,10.37,0.05,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 20260519.2895 10.37CV 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 19.2895 2461179.7895 10.55 22:21:27.93 +33:16:36.4
90.17115 -19.88682 galactic Peg Second-epoch detections are separated by 4.5" and 0.9 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 J335.3615+33.2799 | 22:21:27.93 +33:16:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.668+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:27.93 +33:16:36.4: 11.82 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:27.93 +33:16:36.4: 13.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 J335.3615+33.2799,2461179.7895,10.55,0.05,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
ATO J335.3615+33.2799 20260519.2895 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 19.2895 2461179.7895 10.98 21:33:38.33 +37:37:18.2
85.21073 -10.36551 galactic Cyg Second-epoch detections are separated by 1.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:38.33 +37:37:18.2 (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 21:33:38.33 +37:37:18.2: 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 21:33:38.33 +37:37:18.2: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 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,2461179.7895,10.98,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.94 21:31:28.39 +35:34:31.0
83.44936 -11.54301 galactic Cyg Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8685+35.5755 | 21:31:29.78 +35:35:00.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.195+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:28.39 +35:34:31.0: 11.87 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:28.39 +35:34:31.0: 13.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 J322.8685+35.5755,2461179.7895,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.8685+35.5755 20260519.2895 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.56 22:21:20.67 +32:54:29.7
89.92287 -20.17325 galactic Peg Second-epoch detections are separated by 1.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:20.67 +32:54:29.7 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.024 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:20.67 +32:54:29.7: 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 22:21:20.67 +32:54:29.7: 13.67 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461179.7895,10.56,0.05,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
target 20260519.2895 10.56CV 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 19.2895 2461179.7895 10.46 22:21:52.14 +33:11:04.7
90.18813 -20.01073 galactic Peg Second-epoch detections are separated by 3.2" and 1.2 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 1902046887175458176 | 22:21:52.20 +33:11:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.226+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:52.14 +33:11:04.7: 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 22:21:52.14 +33:11:04.7: 13.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 1902046887175458176,2461179.7895,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902046887175458176 20260519.2895 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.61 22:22:16.23 +33:18:12.1
90.33381 -19.96178 galactic Peg Second-epoch detections are separated by 1.2" and 1.6 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 J335.5695+33.3021 | 22:22:16.23 +33:18:12.1 (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 22:22:16.23 +33:18:12.1: 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 22:22:16.23 +33:18:12.1: 14.05 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.05 +/- 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
ATO J335.5695+33.3021,2461179.7895,10.61,0.05,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
ATO J335.5695+33.3021 20260519.2895 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 19.2895 2461179.7895 10.48 22:22:03.92 +33:34:38.6
90.46363 -19.71276 galactic Peg Second-epoch detections are separated by 2.5" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:03.92 +33:34:38.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.561+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:03.92 +33:34:38.6: 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 22:22:03.92 +33:34:38.6: 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
target,2461179.7895,10.48,0.05,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
target 20260519.2895 10.48CV 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 19.2895 2461179.7895 11.05 21:33:55.65 +39:39:30.3
86.66875 -8.92146 galactic Cyg Second-epoch detections are separated by 0.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1965930574338600448 | 21:33:53.77 +39:39:39.4 (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 21:33:55.65 +39:39:30.3: 11.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:55.65 +39:39:30.3: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965930574338600448,2461179.7895,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965930574338600448 20260519.2895 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.47 22:25:05.76 +34:12:57.2
91.39825 -19.54467 galactic Peg Second-epoch detections are separated by 1.5" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J336.2771+34.2191 | 22:25:05.76 +34:12:57.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:05.76 +34:12:57.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:05.76 +34:12:57.2: 13.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 J336.2771+34.2191,2461179.7895,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J336.2771+34.2191 20260519.2895 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.41 22:21:27.95 +33:30:51.2
90.31649 -19.69271 galactic Peg Second-epoch detections are separated by 0.3" and 1.6 pix
The object was found in VSX19" Gaia DR3 1905069513359948800
Type:
# Max. Min./Amp. JD0 Period
14.070 G 14.110 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 22:21:27.95 +33:30:51.2: 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 22:21:27.95 +33:30:51.2: 13.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 1905069513359948800,2461179.7895,10.41,0.05,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 1905069513359948800 20260519.2895 10.41CV 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 19.2895 2461179.7895 10.48 22:22:33.50 +33:44:26.3
90.65222 -19.63764 galactic Peg Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:33.50 +33:44:26.3 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:33.50 +33:44:26.3: 12.84 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:33.50 +33:44:26.3: 13.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.40 +/- 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,2461179.7895,10.48,0.05,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
target 20260519.2895 10.48CV 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 19.2895 2461179.7895 10.48 22:22:09.47 +32:46:04.4
89.98540 -20.38644 galactic Peg Second-epoch detections are separated by 2.5" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901981225715489408 | 22:22:09.33 +32:46:08.0 (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 22:22:09.47 +32:46:04.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:09.47 +32:46:04.4: 13.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 1901981225715489408,2461179.7895,10.48,0.05,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
Gaia DR3 1901981225715489408 20260519.2895 10.48CV 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 19.2895 2461179.7895 10.54 22:22:40.12 +33:47:33.4
90.70372 -19.60809 galactic Peg Second-epoch detections are separated by 3.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:40.12 +33:47:33.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.298+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:40.12 +33:47:33.4: 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 22:22:40.12 +33:47:33.4: 13.67 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461179.7895,10.54,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.48 22:23:52.63 +33:08:36.3
90.53007 -20.28509 galactic Peg Second-epoch detections are separated by 2.9" and 1.6 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 | 22:23:52.63 +33:08:36.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:52.63 +33:08:36.3: 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 22:23:52.63 +33:08:36.3: 13.68 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 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,2461179.7895,10.48,0.05,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
target 20260519.2895 10.48CV 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 19.2895 2461179.7895 10.46 22:21:41.06 +32:47:20.1
89.91157 -20.31190 galactic Peg Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:41.06 +32:47:20.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:41.06 +32:47:20.1: 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 22:21:41.06 +32:47:20.1: 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,2461179.7895,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.49 22:21:35.28 +33:45:23.8
90.48647 -19.50899 galactic Peg Second-epoch detections are separated by 1.1" and 1.4 pix
The object was found in VSX 6" Gaia DR3 1905170427911132160
Type: ROT
# Max. Min./Amp. JD0 Period
13.960 G 14.000 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 22:21:35.28 +33:45:23.8: 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 22:21:35.28 +33:45:23.8: 13.57 +/- 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 1905170427911132160,2461179.7895,10.49,0.05,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
Gaia DR3 1905170427911132160 20260519.2895 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 19.2895 2461179.7895 10.41 22:24:13.04 +33:46:11.5
90.97109 -19.80988 galactic Peg Second-epoch detections are separated by 1.3" and 1.6 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 | 22:24:13.04 +33:46:11.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:13.04 +33:46:11.5: 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 22:24:13.04 +33:46:11.5: 13.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461179.7895,10.41,0.05,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
target 20260519.2895 10.41CV 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 19.2895 2461179.7895 10.55 22:18:32.61 +32:45:57.5
89.32527 -19.94675 galactic Peg Second-epoch detections are separated by 3.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.6382+32.7685 | 22:18:32.61 +32:45:57.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:32.61 +32:45:57.5: 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 22:18:32.61 +32:45:57.5: 13.32 +/- 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 J334.6382+32.7685,2461179.7895,10.55,0.05,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
ATO J334.6382+32.7685 20260519.2895 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 19.2895 2461179.7895 10.53 22:24:02.73 +34:10:38.8
91.18501 -19.45379 galactic Peg Second-epoch detections are separated by 0.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:02.73 +34:10:38.8 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.029 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:02.73 +34:10:38.8: 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 22:24:02.73 +34:10:38.8: 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,2461179.7895,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.55 22:23:56.54 +33:46:36.7
90.92528 -19.77170 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:56.54 +33:46:36.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.729+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:56.54 +33:46:36.7: 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 22:23:56.54 +33:46:36.7: 13.51 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461179.7895,10.55,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.60 22:20:22.16 +33:02:14.8
89.82489 -19.94953 galactic Peg Second-epoch detections are separated by 1.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:20:22.16 +33:02:14.8 (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 22:20:22.16 +33:02:14.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:22.16 +33:02:14.8: 13.66 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461179.7895,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.51 22:21:22.26 +32:51:29.8
89.89695 -20.21726 galactic Peg Second-epoch detections are separated by 1.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902033074560505600 | 22:21:22.19 +32:51:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.667+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:22.26 +32:51:29.8: 13.33 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:22.26 +32:51:29.8: 13.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 1902033074560505600,2461179.7895,10.51,0.05,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
Gaia DR3 1902033074560505600 20260519.2895 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 19.2895 2461179.7895 11.01 21:16:00.24 +33:40:28.9
79.79649 -10.60212 galactic Cyg Second-epoch detections are separated by 2.3" and 1.8 pix
The object was found in VSX 4" Gaia DR3 1854878972222727808
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.540 G 13.570 G 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 21:16:00.24 +33:40:28.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:00.24 +33:40:28.9: 13.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 1854878972222727808,2461179.7895,11.01,0.05,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 1854878972222727808 20260519.2895 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 19.2895 2461179.7895 10.71 22:23:22.81 +32:55:55.3
90.31019 -20.39925 galactic Peg Second-epoch detections are separated by 1.9" and 1.2 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 | 22:23:22.81 +32:55:55.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.682+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:22.81 +32:55:55.3: 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 22:23:22.81 +32:55:55.3: 13.93 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461179.7895,10.71,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.59 22:24:16.55 +32:44:05.8
90.35508 -20.66846 galactic Peg Second-epoch detections are separated by 1.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:16.55 +32:44:05.8 (user input) | T | P | (position from user input) J-Ks=0.647+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:16.55 +32:44:05.8: 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 22:24:16.55 +32:44:05.8: 13.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461179.7895,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.10 21:20:52.06 +38:17:40.1
83.87011 -8.12087 galactic Cyg Second-epoch detections are separated by 1.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 21:20:52.06 +38:17:40.1: 11.82 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:52.06 +38:17:40.1: 13.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 1964847898984320640,2461179.7895,11.10,0.05,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
Gaia DR3 1964847898984320640 20260519.2895 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 19.2895 2461179.7895 11.05 21:25:56.61 +38:11:59.4
84.51266 -8.89435 galactic Cyg Second-epoch detections are separated by 0.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1964423968521888896 | 21:25:54.24 +38:12:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.930+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:56.61 +38:11:59.4: 13.12 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:56.61 +38:11:59.4: 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
Gaia DR3 1964423968521888896,2461179.7895,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964423968521888896 20260519.2895 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.96 21:39:42.01 +39:56:25.6
87.68892 -9.46433 galactic Cyg Second-epoch detections are separated by 4.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:42.01 +39:56:25.6 (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 21:39:42.01 +39:56:25.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:42.01 +39:56:25.6: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 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,2461179.7895,10.96,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.28 21:14:44.97 +38:12:04.6
82.96245 -7.31926 galactic Cyg Second-epoch detections are separated by 1.4" and 1.2 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 J318.6921+38.2089 | 21:14:44.97 +38:12:04.6 (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 21:14:44.97 +38:12:04.6: 12.55 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:44.97 +38:12:04.6: 13.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.29 +/- 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+38.2089,2461179.7895,11.28,0.05,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 J318.6921+38.2089 20260519.2895 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 19.2895 2461179.7895 10.61 22:20:40.46 +33:17:26.4
90.03613 -19.78005 galactic Peg Second-epoch detections are separated by 2.9" and 1.6 pix
The object was found in VSX 2" ASASSN-V J222040.52+331728.6
Type: EA
# Max. Min./Amp. JD0 Period
12.750 V 13.550 V 2457323.80000 8.236900000000
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 22:20:40.46 +33:17:26.4: 11.61 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:40.46 +33:17:26.4: 13.59 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.45 +/- 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
ASASSN-V J222040.52+331728.6,2461179.7895,10.61,0.05,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
ASASSN-V J222040.52+331728.6 20260519.2895 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 19.2895 2461179.7895 10.53 22:21:08.78 +32:46:19.5
89.80280 -20.26031 galactic Peg Second-epoch detections are separated by 2.5" and 1.2 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 | 22:21:08.78 +32:46:19.5 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.024 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:08.78 +32:46:19.5: 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 22:21:08.78 +32:46:19.5: 13.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.42 +/- 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,2461179.7895,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.90 21:58:07.65 +38:56:43.1
89.79237 -12.52720 galactic Lac Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:07.65 +38:56:43.1 (user input) | T | P | (position from user input) J-Ks=0.794+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:07.65 +38:56:43.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:07.65 +38:56:43.1: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 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,2461179.7895,10.90,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.67 22:21:26.71 +33:33:54.4
90.34384 -19.64861 galactic Peg Second-epoch detections are separated by 1.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:26.71 +33:33:54.4 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:26.71 +33:33:54.4: 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 22:21:26.71 +33:33:54.4: 13.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461179.7895,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.65 22:20:56.51 +33:12:56.9
90.03864 -19.87346 galactic Peg Second-epoch detections are separated by 1.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:20:56.51 +33:12:56.9 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:56.51 +33:12:56.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:56.51 +33:12:56.9: 13.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461179.7895,10.65,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.55 22:23:24.36 +33:31:45.1
90.67796 -19.91196 galactic Peg Second-epoch detections are separated by 3.0" and 1.2 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 1902151650017151872 | 22:23:24.38 +33:31:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.845+/-0.025 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:24.36 +33:31:45.1: 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 22:23:24.36 +33:31:45.1: 13.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 1902151650017151872,2461179.7895,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902151650017151872 20260519.2895 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 19.2895 2461179.7895 10.62 22:22:39.66 +33:39:09.3
90.61738 -19.72210 galactic Peg Second-epoch detections are separated by 2.3" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:39.66 +33:39:09.3 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:39.66 +33:39:09.3: 12.48 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:39.66 +33:39:09.3: 13.63 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.40 +/- 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,2461179.7895,10.62,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.01 21:35:16.60 +37:59:52.8
85.71233 -10.31317 galactic Cyg Second-epoch detections are separated by 2.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.8033+37.9992 | 21:35:16.60 +37:59:52.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.419+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:16.60 +37:59:52.8: 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 21:35:16.60 +37:59:52.8: 13.26 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 J323.8033+37.9992,2461179.7895,11.01,0.05,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
ATO J323.8033+37.9992 20260519.2895 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 19.2895 2461179.7895 10.56 22:22:56.58 +33:21:10.8
90.48660 -20.00153 galactic Peg Second-epoch detections are separated by 4.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:56.58 +33:21:10.8 (user input) | T | P | (position from user input) J-Ks=0.670+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:56.58 +33:21:10.8: 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 22:22:56.58 +33:21:10.8: 13.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461179.7895,10.56,0.05,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
target 20260519.2895 10.56CV 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 19.2895 2461179.7895 10.63 22:24:48.21 +34:20:20.0
91.41875 -19.40900 galactic Peg Second-epoch detections are separated by 1.3" and 1.6 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 | 22:24:48.21 +34:20:20.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.612+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:48.21 +34:20:20.0: 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 22:24:48.21 +34:20:20.0: 13.69 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461179.7895,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.56 22:24:35.00 +33:07:57.2
90.65317 -20.37807 galactic Peg Second-epoch detections are separated by 1.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J336.1453+33.1305 | 22:24:35.00 +33:07:57.2 (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 22:24:35.00 +33:07:57.2: 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 22:24:35.00 +33:07:57.2: 13.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 J336.1453+33.1305,2461179.7895,10.56,0.05,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
ATO J336.1453+33.1305 20260519.2895 10.56CV 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 19.2895 2461179.7895 10.61 22:21:43.44 +33:19:20.4
90.24600 -19.88066 galactic Peg Second-epoch detections are separated by 1.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:43.44 +33:19:20.4 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.027 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:43.44 +33:19:20.4: 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 22:21:43.44 +33:19:20.4: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 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,2461179.7895,10.61,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.70 22:22:59.31 +33:34:17.8
90.62770 -19.82751 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:59.31 +33:34:17.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.787+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:59.31 +33:34:17.8: 12.67 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:59.31 +33:34:17.8: 13.70 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.49 +/- 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,2461179.7895,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.93 22:01:53.20 +40:17:20.1
91.22543 -11.92080 galactic Lac Second-epoch detections are separated by 1.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959629032677924224 | 22:01:56.52 +40:17:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.006+/-0.038 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:53.20 +40:17:20.1: 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 22:01:53.20 +40:17:20.1: 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
Gaia DR3 1959629032677924224,2461179.7895,10.93,0.05,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
Gaia DR3 1959629032677924224 20260519.2895 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 19.2895 2461179.7895 10.51 22:24:26.90 +33:02:13.5
90.57048 -20.44060 galactic Peg Second-epoch detections are separated by 1.4" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902073997008517248 | 22:24:26.86 +33:02:14.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.701+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:26.90 +33:02:13.5: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:26.90 +33:02:13.5: 13.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 1902073997008517248,2461179.7895,10.51,0.05,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
Gaia DR3 1902073997008517248 20260519.2895 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 19.2895 2461179.7895 10.57 22:23:34.30 +33:56:59.1
90.96226 -19.58569 galactic Peg Second-epoch detections are separated by 2.0" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:34.30 +33:56:59.1 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.027 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:34.30 +33:56:59.1: 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 22:23:34.30 +33:56:59.1: 13.63 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461179.7895,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.65 22:18:13.04 +32:48:49.6
89.29600 -19.86784 galactic Peg Second-epoch detections are separated by 1.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:13.04 +32:48:49.6 (user input) | T | P | (position from user input) J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:13.04 +32:48:49.6: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:13.04 +32:48:49.6: 13.67 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461179.7895,10.65,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.67 22:23:41.27 +33:35:11.1
90.76394 -19.89834 galactic Peg Second-epoch detections are separated by 4.5" and 1.0 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 | 22:23:41.27 +33:35:11.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:41.27 +33:35:11.1: 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 22:23:41.27 +33:35:11.1: 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,2461179.7895,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.89 22:19:37.58 +42:13:56.2
95.15176 -12.30556 galactic Lac Second-epoch detections are separated by 3.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1958517701299225088 | 22:19:36.48 +42:14:29.8 (Gaia DR3) | S (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 22:19:37.58 +42:13:56.2: 11.60 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:37.58 +42:13:56.2: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.48 +/- 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 1958517701299225088,2461179.7895,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958517701299225088 20260519.2895 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.70 22:22:30.21 +33:34:23.6
90.54058 -19.76845 galactic Peg Second-epoch detections are separated by 2.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:30.21 +33:34:23.6 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:30.21 +33:34:23.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:30.21 +33:34:23.6: 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
target,2461179.7895,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.67 22:23:03.75 +33:14:11.5
90.43753 -20.11137 galactic Peg Second-epoch detections are separated by 2.3" and 1.6 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 | 22:23:03.75 +33:14:11.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:03.75 +33:14:11.5: 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 22:23:03.75 +33:14:11.5: 13.83 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461179.7895,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.84 22:24:57.77 +33:32:13.7
90.96702 -20.08954 galactic Peg Second-epoch detections are separated by 1.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:57.77 +33:32:13.7 (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 22:24:57.77 +33:32:13.7: 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 22:24:57.77 +33:32:13.7: 13.62 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461179.7895,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.63 22:23:10.70 +33:50:35.1
90.82659 -19.62700 galactic Peg Second-epoch detections are separated by 0.7" and 1.6 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 | 22:23:10.70 +33:50:35.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:10.70 +33:50:35.1: 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 22:23:10.70 +33:50:35.1: 13.83 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461179.7895,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.66 22:24:39.03 +33:58:16.5
91.17093 -19.69470 galactic Peg Second-epoch detections are separated by 1.8" and 1.6 pix
The object was found in VSX 6" Gaia DR3 1902199891090067072
Type: ROT
# Max. Min./Amp. JD0 Period
14.700 G 14.730 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 22:24:39.03 +33:58:16.5: 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 22:24:39.03 +33:58:16.5: 13.72 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 1902199891090067072,2461179.7895,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902199891090067072 20260519.2895 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.16 21:25:05.62 +37:46:27.9
84.08879 -9.07803 galactic Cyg Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.2679+37.7763 | 21:25:05.62 +37:46:27.9 (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 21:25:05.62 +37:46:27.9: 12.40 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:05.62 +37:46:27.9: 13.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 J321.2679+37.7763,2461179.7895,11.16,0.05,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
ATO J321.2679+37.7763 20260519.2895 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 19.2895 2461179.7895 10.63 22:22:12.35 +33:29:02.2
90.43219 -19.80610 galactic Peg Second-epoch detections are separated by 2.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:12.35 +33:29:02.2 (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 22:22:12.35 +33:29:02.2: 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 22:22:12.35 +33:29:02.2: 13.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461179.7895,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.00 21:42:06.09 +36:50:54.1
85.93752 -12.07632 galactic Cyg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5190+36.8572 | 21:42:02.55 +36:51:12.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:06.09 +36:50:54.1: 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 21:42:06.09 +36:50:54.1: 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 J325.5190+36.8572,2461179.7895,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5190+36.8572 20260519.2895 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.74 22:21:30.33 +33:21:21.8
90.22695 -19.82682 galactic Peg Second-epoch detections are separated by 2.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:30.33 +33:21:21.8 (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 22:21:30.33 +33:21:21.8: 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 22:21:30.33 +33:21:21.8: 13.73 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461179.7895,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.25 21:18:35.27 +40:16:40.9
84.99113 -6.42011 galactic Cyg Second-epoch detections are separated by 4.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.6471+40.2846 | 21:18:33.06 +40:16:53.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.535+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:35.27 +40:16:40.9: 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 21:18:35.27 +40:16:40.9: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.10 +/- 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+40.2846,2461179.7895,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.6471+40.2846 20260519.2895 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.74 22:23:37.08 +34:04:43.8
91.04842 -19.48489 galactic Peg Second-epoch detections are separated by 2.1" and 1.2 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 | 22:23:37.08 +34:04:43.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.576+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:37.08 +34:04:43.8: 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 22:23:37.08 +34:04:43.8: 13.70 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461179.7895,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.68 22:19:38.04 +33:02:55.3
89.69844 -19.85086 galactic Peg Second-epoch detections are separated by 0.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.9089+33.0488 | 22:19:38.04 +33:02:55.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.509+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:38.04 +33:02:55.3: 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 22:19:38.04 +33:02:55.3: 13.80 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 J334.9089+33.0488,2461179.7895,10.68,0.05,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 J334.9089+33.0488 20260519.2895 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 19.2895 2461179.7895 10.81 22:21:05.10 +33:08:35.2
90.01999 -19.95010 galactic Peg Second-epoch detections are separated by 1.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:05.10 +33:08:35.2 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:05.10 +33:08:35.2: 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 22:21:05.10 +33:08:35.2: 13.66 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461179.7895,10.81,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.29 21:10:36.29 +40:19:48.4
83.97649 -5.27979 galactic Cyg Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:36.29 +40:19:48.4 (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 21:10:36.29 +40:19:48.4: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:36.29 +40:19:48.4: 13.62 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461179.7895,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.69 22:17:57.51 +33:00:25.5
89.36976 -19.67942 galactic Peg Second-epoch detections are separated by 2.2" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:57.51 +33:00:25.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) 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 22:17:57.51 +33:00:25.5: 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 22:17:57.51 +33:00:25.5: 13.74 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461179.7895,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.90 21:57:40.58 +37:18:46.3
88.66911 -13.74221 galactic Cyg Second-epoch detections are separated by 2.7" and 1.6 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 J329.4294+37.3037 | 21:57:40.58 +37:18:46.3 (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 21:57:40.58 +37:18:46.3: 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 21:57:40.58 +37:18:46.3: 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 J329.4294+37.3037,2461179.7895,10.90,0.05,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
ATO J329.4294+37.3037 20260519.2895 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 19.2895 2461179.7895 10.65 22:21:11.00 +32:48:09.8
89.82845 -20.23982 galactic Peg Second-epoch detections are separated by 2.6" and 1.2 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 | 22:21:11.00 +32:48:09.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.708+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:11.00 +32:48:09.8: 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 22:21:11.00 +32:48:09.8: 13.79 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461179.7895,10.65,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.70 22:23:23.41 +33:32:22.9
90.68144 -19.90146 galactic Peg Second-epoch detections are separated by 3.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902151650017151872 | 22:23:24.38 +33:31:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.254+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:23.41 +33:32:22.9: 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 22:23:23.41 +33:32:22.9: 13.48 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 1902151650017151872,2461179.7895,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902151650017151872 20260519.2895 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.69 22:18:18.44 +33:03:09.3
89.46100 -19.68542 galactic Peg Second-epoch detections are separated by 1.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.5773+33.0529 | 22:18:18.44 +33:03:09.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.566+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:18.44 +33:03:09.3: 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 22:18:18.44 +33:03:09.3: 13.79 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 J334.5773+33.0529,2461179.7895,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.5773+33.0529 20260519.2895 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.61 22:25:06.51 +33:54:39.9
91.21818 -19.79797 galactic Peg Second-epoch detections are separated by 2.2" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:25:06.51 +33:54:39.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.329+/-0.024 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:06.51 +33:54:39.9: 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 22:25:06.51 +33:54:39.9: 13.67 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461179.7895,10.61,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.18 21:42:46.24 +37:59:51.7
86.82189 -11.30909 galactic Cyg Second-epoch detections are separated by 2.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6883+38.0053 | 21:42:43.15 +38:00:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:46.24 +37:59:51.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:46.24 +37:59:51.7: 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
ATO J325.6883+38.0053,2461179.7895,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6883+38.0053 20260519.2895 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.12 21:27:41.86 +38:45:47.5
85.16015 -8.73363 galactic Cyg Second-epoch detections are separated by 3.3" and 1.1 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 J321.9265+38.7675 | 21:27:41.86 +38:45:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.638+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:41.86 +38:45:47.5: 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 21:27:41.86 +38:45:47.5: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 J321.9265+38.7675,2461179.7895,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.9265+38.7675 20260519.2895 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.60 22:23:40.39 +33:06:46.4
90.47410 -20.28583 galactic Peg Second-epoch detections are separated by 1.7" and 1.6 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 | 22:23:40.39 +33:06:46.4 (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 22:23:40.39 +33:06:46.4: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:40.39 +33:06:46.4: 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,2461179.7895,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.64 22:21:28.32 +33:30:23.0
90.31281 -19.69986 galactic Peg Second-epoch detections are separated by 1.4" and 1.8 pix
The object was found in VSX 2" 1SWASP J222128.41+333020.9
Type: EA
# Max. Min./Amp. JD0 Period
12.150 CV 12.350 CV 0.945691500000
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 22:21:28.32 +33:30:23.0: 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 22:21:28.32 +33:30:23.0: 13.98 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
1SWASP J222128.41+333020.9,2461179.7895,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
1SWASP J222128.41+333020.9 20260519.2895 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.63 22:24:04.84 +32:52:51.7
90.40799 -20.52504 galactic Peg Second-epoch detections are separated by 1.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902068602529462400 | 22:24:04.72 +32:52:53.3 (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 22:24:04.84 +32:52:51.7: 13.01 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:04.84 +32:52:51.7: 13.73 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 1902068602529462400,2461179.7895,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902068602529462400 20260519.2895 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.24 21:20:38.11 +36:33:48.2
82.58364 -9.29636 galactic Cyg Second-epoch detections are separated by 4.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.1602+36.5681 | 21:20:38.11 +36:33:48.2 (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 21:20:38.11 +36:33:48.2: 11.70 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:38.11 +36:33:48.2: 13.13 +/- 0.05 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
ATO J320.1602+36.5681,2461179.7895,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.1602+36.5681 20260519.2895 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 19.2895 2461179.7895 10.77 22:22:28.49 +33:51:41.7
90.71048 -19.52848 galactic Peg Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:28.49 +33:51:41.7 (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 22:22:28.49 +33:51:41.7: 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 22:22:28.49 +33:51:41.7: 13.91 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461179.7895,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.07 22:00:54.44 +41:16:16.1
91.69111 -11.03150 galactic Lac Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:54.44 +41:16:16.1 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.044 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:54.44 +41:16:16.1: 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 22:00:54.44 +41:16:16.1: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461179.7895,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.74 22:23:44.96 +32:47:18.9
90.29063 -20.56127 galactic Peg Second-epoch detections are separated by 3.6" and 1.2 pix
The object was found in VSX 3" Gaia DR3 1901973975810832512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.870 G 12.950 G 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 22:23:44.96 +32:47:18.9: 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 22:23:44.96 +32:47:18.9: 14.02 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.02 +/- 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
Gaia DR3 1901973975810832512,2461179.7895,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901973975810832512 20260519.2895 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.82 22:24:08.27 +33:27:45.7
90.77123 -20.05344 galactic Peg Second-epoch detections are separated by 3.0" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:08.27 +33:27:45.7 (user input) | T | P | (position from user input) J-Ks=0.735+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:08.27 +33:27:45.7: 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 22:24:08.27 +33:27:45.7: 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
target,2461179.7895,10.82,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.73 22:25:04.56 +33:47:39.0
91.14216 -19.89072 galactic Peg Second-epoch detections are separated by 0.9" and 1.6 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 | 22:25:04.56 +33:47:39.0 (user input) | T | P | (position from user input) J-Ks=0.702+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:04.56 +33:47:39.0: 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 22:25:04.56 +33:47:39.0: 13.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461179.7895,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.75 22:19:40.49 +33:14:50.8
89.82865 -19.69415 galactic Peg Second-epoch detections are separated by 1.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:40.49 +33:14:50.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.213+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:40.49 +33:14:50.8: 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 22:19:40.49 +33:14:50.8: 13.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461179.7895,10.75,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.73 22:22:31.67 +32:40:34.0
89.99699 -20.50627 galactic Peg Second-epoch detections are separated by 2.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:31.67 +32:40:34.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:31.67 +32:40:34.0: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:31.67 +32:40:34.0: 13.81 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461179.7895,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.35 21:29:07.96 +42:01:04.7
87.64249 -6.58506 galactic Cyg Second-epoch detections are separated by 1.8" and 1.6 pix
The object was found in VSX 5" 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 21:29:07.96 +42:01:04.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:07.96 +42:01:04.7: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 1967190545946435712,2461179.7895,11.35,0.05,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
Gaia DR3 1967190545946435712 20260519.2895 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 19.2895 2461179.7895 10.87 22:18:42.70 +33:05:54.4
89.56246 -19.69777 galactic Peg Second-epoch detections are separated by 2.4" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:42.70 +33:05:54.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:42.70 +33:05:54.4: 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 22:18:42.70 +33:05:54.4: 13.66 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461179.7895,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.77 22:19:54.91 +32:47:47.2
89.59332 -20.09034 galactic Peg Second-epoch detections are separated by 0.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:54.91 +32:47:47.2 (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 22:19:54.91 +32:47:47.2: 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 22:19:54.91 +32:47:47.2: 13.73 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461179.7895,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.71 22:20:47.78 +33:26:03.8
90.14645 -19.67747 galactic Peg Second-epoch detections are separated by 0.5" and 1.6 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 J335.1970+33.4315 | 22:20:47.78 +33:26:03.8 (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 22:20:47.78 +33:26:03.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:47.78 +33:26:03.8: 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
ATO J335.1970+33.4315,2461179.7895,10.71,0.05,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
ATO J335.1970+33.4315 20260519.2895 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 19.2895 2461179.7895 11.19 22:02:42.37 +41:44:11.1
92.25230 -10.86919 galactic Lac Second-epoch detections are separated by 1.4" and 1.6 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 1959859277284333312 | 22:02:40.01 +41:44:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.37 +41:44:11.1: 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 22:02:42.37 +41:44:11.1: 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
Gaia DR3 1959859277284333312,2461179.7895,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959859277284333312 20260519.2895 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 19.2895 2461179.7895 10.82 22:22:23.71 +32:51:01.8
90.07960 -20.34754 galactic Peg Second-epoch detections are separated by 1.3" and 1.5 pix
The object was found in VSX 4" Gaia DR3 1901985967359952896
Type: ROT
# Max. Min./Amp. JD0 Period
12.740 G 12.790 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 22:22:23.71 +32:51:01.8: 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 22:22:23.71 +32:51:01.8: 13.87 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.87 +/- 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
Gaia DR3 1901985967359952896,2461179.7895,10.82,0.05,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
Gaia DR3 1901985967359952896 20260519.2895 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 19.2895 2461179.7895 11.29 21:29:04.91 +40:27:04.7
86.54141 -7.70798 galactic Cyg Second-epoch detections are separated by 2.3" and 1.0 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 J322.2754+40.4518 | 21:29:04.91 +40:27:04.7 (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 21:29:04.91 +40:27:04.7: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:04.91 +40:27:04.7: 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+40.4518,2461179.7895,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.2754+40.4518 20260519.2895 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.68 22:19:44.20 +32:47:01.0
89.55289 -20.07894 galactic Peg Second-epoch detections are separated by 4.5" and 1.6 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 J334.9351+32.7831 | 22:19:44.20 +32:47:01.0 (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 22:19:44.20 +32:47:01.0: 13.03 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:44.20 +32:47:01.0: 13.77 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 J334.9351+32.7831,2461179.7895,10.68,0.05,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 J334.9351+32.7831 20260519.2895 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 19.2895 2461179.7895 11.29 21:12:50.82 +36:08:09.5
81.17774 -8.45239 galactic Cyg Second-epoch detections are separated by 0.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.2116+36.1294 | 21:12:48.44 +36:07:43.1 (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 21:12:50.82 +36:08:09.5: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:50.82 +36:08:09.5: 13.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 J318.2116+36.1294,2461179.7895,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.2116+36.1294 20260519.2895 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.88 22:25:35.96 +34:15:30.1
91.51489 -19.56802 galactic Peg Second-epoch detections are separated by 2.0" and 1.2 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 | 22:25:35.96 +34:15:30.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.242+/-0.029 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:35.96 +34:15:30.1: 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 22:25:35.96 +34:15:30.1: 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,2461179.7895,10.88,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.68 22:23:36.74 +33:59:16.9
90.99270 -19.55898 galactic Peg Second-epoch detections are separated by 2.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:36.74 +33:59:16.9 (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 22:23:36.74 +33:59:16.9: 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 22:23:36.74 +33:59:16.9: 14.03 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461179.7895,10.68,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.82 22:21:41.54 +33:58:45.2
90.64073 -19.33910 galactic Peg Second-epoch detections are separated by 2.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:41.54 +33:58:45.2 (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 22:21:41.54 +33:58:45.2: 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 22:21:41.54 +33:58:45.2: 13.80 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461179.7895,10.82,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.81 22:23:22.96 +33:18:06.0
90.53565 -20.09611 galactic Peg Second-epoch detections are separated by 2.1" and 1.6 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 | 22:23:22.96 +33:18:06.0 (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 22:23:22.96 +33:18:06.0: 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 22:23:22.96 +33:18:06.0: 13.67 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461179.7895,10.81,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.71 22:23:49.40 +33:29:56.6
90.73579 -19.98626 galactic Peg Second-epoch detections are separated by 2.6" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:49.40 +33:29:56.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.573+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:49.40 +33:29:56.6: 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 22:23:49.40 +33:29:56.6: 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,2461179.7895,10.71,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.36 21:34:28.18 +39:24:27.9
86.57259 -9.17591 galactic Cyg Second-epoch detections are separated by 1.6" and 1.2 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 1965875972415567488 | 21:34:26.01 +39:24:24.7 (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 21:34:28.18 +39:24:27.9: 12.96 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:28.18 +39:24:27.9: 13.50 +/- 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
Gaia DR3 1965875972415567488,2461179.7895,11.36,0.05,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 1965875972415567488 20260519.2895 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 19.2895 2461179.7895 10.79 22:24:01.94 +33:34:40.3
90.82156 -19.94616 galactic Peg Second-epoch detections are separated by 4.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:01.94 +33:34:40.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:01.94 +33:34:40.3: 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 22:24:01.94 +33:34:40.3: 13.77 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461179.7895,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.22 22:00:15.54 +42:40:25.6
92.46996 -9.85029 galactic Lac Second-epoch detections are separated by 1.2" and 1.2 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 | 22:00:15.54 +42:40:25.6 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:15.54 +42:40:25.6: 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 22:00:15.54 +42:40:25.6: 13.71 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461179.7895,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.82 22:20:18.57 +32:56:13.8
89.75211 -20.02393 galactic Peg Second-epoch detections are separated by 1.4" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:20:18.57 +32:56:13.8 (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 22:20:18.57 +32:56:13.8: 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 22:20:18.57 +32:56:13.8: 13.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461179.7895,10.82,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.81 22:24:19.50 +33:47:17.9
91.00179 -19.80735 galactic Peg Second-epoch detections are separated by 1.2" and 1.6 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 | 22:24:19.50 +33:47:17.9 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:19.50 +33:47:17.9: 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 22:24:19.50 +33:47:17.9: 13.99 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461179.7895,10.81,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.38 21:33:38.97 +39:05:53.5
86.24072 -9.29310 galactic Cyg Second-epoch detections are separated by 0.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4104+39.0760 | 21:33:39.11 +39:05:18.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.398+/-0.057 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:38.97 +39:05:53.5: 12.47 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:38.97 +39:05:53.5: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 J323.4104+39.0760,2461179.7895,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4104+39.0760 20260519.2895 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 19.2895 2461179.7895 11.14 21:49:54.43 +34:54:45.8
85.83894 -14.57367 galactic Peg Second-epoch detections are separated by 2.9" and 1.6 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 | 21:49:54.43 +34:54:45.8 (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 21:49:54.43 +34:54:45.8: 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 21:49:54.43 +34:54:45.8: 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
target,2461179.7895,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.71 22:19:14.02 +32:43:30.4
89.42510 -20.06478 galactic Peg Second-epoch detections are separated by 1.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.8098+32.7280 | 22:19:14.02 +32:43:30.4 (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 22:19:14.02 +32:43:30.4: 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 22:19:14.02 +32:43:30.4: 13.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J334.8098+32.7280,2461179.7895,10.71,0.05,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
ATO J334.8098+32.7280 20260519.2895 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 19.2895 2461179.7895 11.20 21:59:27.31 +38:47:13.7
89.89820 -12.81206 galactic Lac Second-epoch detections are separated by 2.9" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:27.31 +38:47:13.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:27.31 +38:47:13.7: 13.45 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:27.31 +38:47:13.7: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461179.7895,11.20,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.18 22:01:13.39 +38:33:03.0
90.02555 -13.21148 galactic Lac Second-epoch detections are separated by 1.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3009+38.5652 | 22:01:14.28 +38:33:47.5 (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 22:01:13.39 +38:33:03.0: 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 22:01:13.39 +38:33:03.0: 13.62 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 J330.3009+38.5652,2461179.7895,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3009+38.5652 20260519.2895 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.95 22:22:24.25 +33:43:44.1
90.61718 -19.62893 galactic Peg Second-epoch detections are separated by 3.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:24.25 +33:43:44.1 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:24.25 +33:43:44.1: 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 22:22:24.25 +33:43:44.1: 14.07 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461179.7895,10.95,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.82 22:19:18.86 +33:03:23.4
89.64538 -19.80551 galactic Peg Second-epoch detections are separated by 2.6" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:18.86 +33:03:23.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:18.86 +33:03:23.4: 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 22:19:18.86 +33:03:23.4: 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,2461179.7895,10.82,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.07 22:02:42.05 +37:08:58.3
89.37022 -14.49363 galactic Lac Second-epoch detections are separated by 1.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1954935045741178880 | 22:02:43.32 +37:08:15.0 (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 22:02:42.05 +37:08:58.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.05 +37:08:58.3: 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
Gaia DR3 1954935045741178880,2461179.7895,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954935045741178880 20260519.2895 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.12 22:07:49.39 +33:25:38.5
87.84394 -18.07143 galactic Peg Second-epoch detections are separated by 1.9" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9469+33.4302 | 22:07:49.39 +33:25:38.5 (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 22:07:49.39 +33:25:38.5: 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 22:07:49.39 +33:25:38.5: 13.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.70 +/- 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+33.4302,2461179.7895,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9469+33.4302 20260519.2895 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.78 22:22:25.23 +32:47:16.9
90.04594 -20.40172 galactic Peg Second-epoch detections are separated by 3.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.6065+32.7922 | 22:22:25.23 +32:47:16.9 (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 22:22:25.23 +32:47:16.9: 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 22:22:25.23 +32:47:16.9: 14.03 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.03 +/- 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
ATO J335.6065+32.7922,2461179.7895,10.78,0.05,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
ATO J335.6065+32.7922 20260519.2895 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.16 22:04:54.80 +37:38:40.9
90.04227 -14.37246 galactic Lac Second-epoch detections are separated by 2.4" and 1.0 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 | 22:04:54.80 +37:38:40.9 (user input) | T | P | (position from user input) J-Ks=0.543+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:54.80 +37:38:40.9: 13.30 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:54.80 +37:38:40.9: 13.78 +/- 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
target,2461179.7895,11.16,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.38 21:39:02.81 +40:22:36.4
87.89139 -9.05686 galactic Cyg Second-epoch detections are separated by 2.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:02.81 +40:22:36.4 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:02.81 +40:22:36.4: 12.47 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:02.81 +40:22:36.4: 13.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461179.7895,11.38,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.12 21:52:08.98 +36:25:24.0
87.20871 -13.72206 galactic Peg Second-epoch detections are separated by 2.0" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:08.98 +36:25:24.0 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:08.98 +36:25:24.0: 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 21:52:08.98 +36:25:24.0: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461179.7895,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.86 22:22:37.60 +33:42:30.3
90.64504 -19.67220 galactic Peg Second-epoch detections are separated by 1.0" and 1.6 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 | 22:22:37.60 +33:42:30.3 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.645+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:37.60 +33:42:30.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:37.60 +33:42:30.3: 13.99 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461179.7895,10.86,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.08 22:03:59.82 +39:46:39.6
91.23314 -12.57233 galactic Lac Second-epoch detections are separated by 2.3" and 1.6 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 | 22:03:59.82 +39:46:39.6 (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 22:03:59.82 +39:46:39.6: 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 22:03:59.82 +39:46:39.6: 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
target,2461179.7895,11.08,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.33 21:26:13.31 +36:37:42.3
83.42993 -10.04843 galactic Cyg Second-epoch detections are separated by 4.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:26:13.31 +36:37:42.3 (user input) | T | P | (position from user input) J-Ks=0.211+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:13.31 +36:37:42.3: 11.56 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:13.31 +36:37:42.3: 13.57 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.55 +/- 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,2461179.7895,11.33,0.05,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 20260519.2895 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.82 22:23:00.58 +33:18:08.4
90.46794 -20.05106 galactic Peg Second-epoch detections are separated by 1.2" and 1.6 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 | 22:23:00.58 +33:18:08.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:00.58 +33:18:08.4: 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 22:23:00.58 +33:18:08.4: 14.02 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461179.7895,10.82,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.73 22:21:30.45 +33:24:03.5
90.25480 -19.79033 galactic Peg Second-epoch detections are separated by 1.7" and 1.6 pix
The object was found in VSX 2" Gaia DR3 1902065441434285696
Type: ROT
# Max. Min./Amp. JD0 Period
12.780 G 12.800 G 14.957700000000 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 22:21:30.45 +33:24:03.5: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:30.45 +33:24:03.5: 13.76 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 1902065441434285696,2461179.7895,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902065441434285696 20260519.2895 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.88 22:18:38.59 +32:52:57.5
89.41597 -19.86443 galactic Peg Second-epoch detections are separated by 1.0" and 1.6 pix
The object was found in VSX 3" Gaia DR3 1905023952346348544
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.030 G 13.110 G 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 22:18:38.59 +32:52:57.5: 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 22:18:38.59 +32:52:57.5: 13.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 1905023952346348544,2461179.7895,10.88,0.05,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
Gaia DR3 1905023952346348544 20260519.2895 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 19.2895 2461179.7895 10.79 22:21:48.57 +33:16:34.8
90.23341 -19.92857 galactic Peg Second-epoch detections are separated by 3.5" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:48.57 +33:16:34.8 (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 22:21:48.57 +33:16:34.8: 13.17 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:48.57 +33:16:34.8: 13.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461179.7895,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.91 22:22:28.70 +33:12:04.8
90.30942 -20.07028 galactic Peg Second-epoch detections are separated by 1.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:28.70 +33:12:04.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:28.70 +33:12:04.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:28.70 +33:12:04.8: 14.06 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461179.7895,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.02 22:24:30.17 +33:12:13.8
90.68152 -20.30983 galactic Peg Second-epoch detections are separated by 2.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:30.17 +33:12:13.8 (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 22:24:30.17 +33:12:13.8: 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 22:24:30.17 +33:12:13.8: 13.86 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.13 22:06:46.39 +39:39:08.4
91.59135 -12.99506 galactic Lac Second-epoch detections are separated by 2.4" and 1.2 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 | 22:06:46.39 +39:39:08.4 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.641+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:46.39 +39:39:08.4: 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 22:06:46.39 +39:39:08.4: 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,2461179.7895,11.13,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.93 22:23:33.08 +32:55:50.5
90.34083 -20.42087 galactic Peg Second-epoch detections are separated by 4.3" and 0.8 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 | 22:23:33.08 +32:55:50.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:33.08 +32:55:50.5: 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 22:23:33.08 +32:55:50.5: 13.92 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461179.7895,10.93,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.82 22:22:24.55 +33:38:18.5
90.56313 -19.70370 galactic Peg Second-epoch detections are separated by 2.9" and 1.9 pix
The object was found in VSX 1" ZTF J222224.54+333819.4
Type: SR
# Max. Min./Amp. JD0 Period
13.828 g Y 0.298 g 2458306.03720 48.657698500000
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 22:22:24.55 +33:38:18.5: 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 22:22:24.55 +33:38:18.5: 13.79 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.79 +/- 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
ZTF J222224.54+333819.4,2461179.7895,10.82,0.05,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
ZTF J222224.54+333819.4 20260519.2895 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 19.2895 2461179.7895 11.18 21:54:04.33 +37:39:40.0
88.32795 -13.01952 galactic Cyg Second-epoch detections are separated by 3.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.5216+37.6572 | 21:54:04.06 +37:39:00.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:04.33 +37:39:40.0: 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 21:54:04.33 +37:39:40.0: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 J328.5216+37.6572,2461179.7895,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.5216+37.6572 20260519.2895 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.03 22:21:33.24 +33:09:58.7
90.11954 -19.98778 galactic Peg Second-epoch detections are separated by 1.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:33.24 +33:09:58.7 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:33.24 +33:09:58.7: 12.51 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:33.24 +33:09:58.7: 13.91 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.40 +/- 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,2461179.7895,11.03,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.85 22:21:07.02 +32:55:56.2
89.89615 -20.12606 galactic Peg Second-epoch detections are separated by 1.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:07.02 +32:55:56.2 (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 22:21:07.02 +32:55:56.2: 12.40 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:07.02 +32:55:56.2: 13.91 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.35 +/- 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,2461179.7895,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.02 22:20:44.06 +33:02:16.2
89.89146 -19.99353 galactic Peg Second-epoch detections are separated by 4.8" and 1.2 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 | 22:20:44.06 +33:02:16.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.313+/-0.027 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:44.06 +33:02:16.2: 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 22:20:44.06 +33:02:16.2: 14.18 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.02 22:24:02.12 +33:51:15.8
90.98891 -19.71881 galactic Peg Second-epoch detections are separated by 1.2" and 1.6 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 | 22:24:02.12 +33:51:15.8 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.027 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:02.12 +33:51:15.8: 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 22:24:02.12 +33:51:15.8: 14.01 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.88 22:19:12.03 +33:10:14.0
89.69542 -19.69893 galactic Peg Second-epoch detections are separated by 1.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:12.03 +33:10:14.0 (user input) | T | P | (position from user input) J-Ks=0.558+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:12.03 +33:10:14.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:12.03 +33:10:14.0: 13.88 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461179.7895,10.88,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.04 22:02:40.27 +38:06:45.8
89.97753 -13.73147 galactic Lac Second-epoch detections are separated by 4.5" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.6734+38.1123 | 22:02:40.27 +38:06:45.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.372+/-0.064 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:40.27 +38:06:45.8: 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 22:02:40.27 +38:06:45.8: 13.72 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 J330.6734+38.1123,2461179.7895,11.04,0.05,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 J330.6734+38.1123 20260519.2895 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 19.2895 2461179.7895 11.25 21:37:56.45 +40:23:15.4
87.74087 -8.90728 galactic Cyg Second-epoch detections are separated by 1.2" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1966025609071043456 | 21:37:58.59 +40:23:14.9 (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 21:37:56.45 +40:23:15.4: 13.03 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:56.45 +40:23:15.4: 13.43 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 1966025609071043456,2461179.7895,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966025609071043456 20260519.2895 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.43 21:36:22.22 +40:35:08.1
87.65321 -8.55964 galactic Cyg Second-epoch detections are separated by 1.6" and 1.1 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 J324.0983+40.5755 | 21:36:22.22 +40:35:08.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.934+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:22.22 +40:35:08.1: 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 21:36:22.22 +40:35:08.1: 13.58 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 J324.0983+40.5755,2461179.7895,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.0983+40.5755 20260519.2895 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.36 21:27:59.75 +37:32:19.5
84.33475 -9.64950 galactic Cyg Second-epoch detections are separated by 0.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:59.75 +37:32:19.5 (user input) | T | P | (position from user input) J-Ks=0.836+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:59.75 +37:32:19.5: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:59.75 +37:32:19.5: 13.68 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 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,2461179.7895,11.36,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.96 22:25:26.04 +34:33:53.2
91.66727 -19.29525 galactic Peg Second-epoch detections are separated by 1.8" and 1.2 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 | 22:25:26.04 +34:33:53.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.274+/-0.026 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:26.04 +34:33:53.2: 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 22:25:26.04 +34:33:53.2: 13.92 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461179.7895,10.96,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.34 21:42:23.04 +40:36:53.8
88.53127 -9.30224 galactic Cyg Second-epoch detections are separated by 3.1" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5857+40.6170 | 21:42:23.04 +40:36:53.8 (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 21:42:23.04 +40:36:53.8: 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 21:42:23.04 +40:36:53.8: 13.72 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 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+40.6170,2461179.7895,11.34,0.05,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 J325.5857+40.6170 20260519.2895 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 19.2895 2461179.7895 11.38 21:40:43.71 +37:23:00.9
86.09657 -11.49569 galactic Cyg Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1759+37.3947 | 21:40:43.71 +37:23:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.217+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:43.71 +37:23:00.9: 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 21:40:43.71 +37:23:00.9: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 J325.1759+37.3947,2461179.7895,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1759+37.3947 20260519.2895 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 19.2895 2461179.7895 11.36 21:35:18.47 +37:59:45.7
85.71551 -10.31880 galactic Cyg Second-epoch detections are separated by 2.8" and 0.9 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 | 21:35:18.47 +37:59:45.7 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:18.47 +37:59:45.7: 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 21:35:18.47 +37:59:45.7: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461179.7895,11.36,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.29 21:44:49.77 +36:56:55.2
86.42218 -12.36468 galactic Cyg Second-epoch detections are separated by 2.0" and 1.2 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 | 21:44:49.77 +36:56:55.2 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:49.77 +36:56:55.2: 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 21:44:49.77 +36:56:55.2: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461179.7895,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.12 22:14:26.75 +39:28:50.0
92.71386 -14.00731 galactic Lac Second-epoch detections are separated by 1.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:14:26.75 +39:28:50.0 (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 22:14:26.75 +39:28:50.0: 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 22:14:26.75 +39:28:50.0: 13.65 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461179.7895,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.91 22:21:28.15 +33:14:45.2
90.15289 -19.91251 galactic Peg Second-epoch detections are separated by 3.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:28.15 +33:14:45.2 (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 22:21:28.15 +33:14:45.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:28.15 +33:14:45.2: 14.04 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461179.7895,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.89 22:21:50.53 +33:31:59.9
90.39631 -19.72218 galactic Peg Second-epoch detections are separated by 1.4" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:50.53 +33:31:59.9 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:50.53 +33:31:59.9: 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 22:21:50.53 +33:31:59.9: 13.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461179.7895,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.21 22:18:43.00 +33:06:49.5
89.57286 -19.68596 galactic Peg Second-epoch detections are separated by 2.3" and 1.5 pix
The object was found in VSX 2" ZTF J221843.12+330650.2
Type: RS
# Max. Min./Amp. JD0 Period
13.288 g Y 0.068 g 2458634.94990 0.459685200000
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 22:18:43.00 +33:06:49.5: 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 22:18:43.00 +33:06:49.5: 13.81 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.81 +/- 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
ZTF J221843.12+330650.2,2461179.7895,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221843.12+330650.2 20260519.2895 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.94 22:23:10.54 +33:38:55.6
90.70851 -19.78636 galactic Peg Second-epoch detections are separated by 2.4" and 1.6 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 | 22:23:10.54 +33:38:55.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:10.54 +33:38:55.6: 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 22:23:10.54 +33:38:55.6: 13.74 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461179.7895,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.02 22:20:27.50 +33:24:46.9
90.07222 -19.65414 galactic Peg Second-epoch detections are separated by 1.6" and 1.3 pix
The object was found in VSX 1" Gaia DR3 1905065149673030656
Type: ROT
# Max. Min./Amp. JD0 Period
13.100 G 13.120 G 0.935300000000 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 22:20:27.50 +33:24:46.9: 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 22:20:27.50 +33:24:46.9: 14.08 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.08 +/- 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
Gaia DR3 1905065149673030656,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905065149673030656 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.96 22:20:27.28 +32:54:53.0
89.76466 -20.05989 galactic Peg Second-epoch detections are separated by 1.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:20:27.28 +32:54:53.0 (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 22:20:27.28 +32:54:53.0: 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 22:20:27.28 +32:54:53.0: 14.30 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461179.7895,10.96,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.38 21:47:33.56 +37:22:57.0
87.13368 -12.39665 galactic Cyg Second-epoch detections are separated by 2.4" and 1.6 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 | 21:47:33.56 +37:22:57.0 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:33.56 +37:22:57.0: 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 21:47:33.56 +37:22:57.0: 13.76 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461179.7895,11.38,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.07 22:22:11.83 +33:26:57.1
90.40943 -19.83354 galactic Peg Second-epoch detections are separated by 1.5" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:22:11.83 +33:26:57.1 (user input) | T | P | (position from user input) J-Ks=0.619+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:11.83 +33:26:57.1: 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 22:22:11.83 +33:26:57.1: 13.89 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461179.7895,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.24 22:04:23.59 +39:34:07.2
91.16489 -12.78460 galactic Lac Second-epoch detections are separated by 2.1" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956534040584630272 | 22:04:23.45 +39:33:43.3 (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 22:04:23.59 +39:34:07.2: 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 22:04:23.59 +39:34:07.2: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 1956534040584630272,2461179.7895,11.24,0.05,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 1956534040584630272 20260519.2895 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 19.2895 2461179.7895 11.00 22:21:49.31 +33:27:50.1
90.35028 -19.77655 galactic Peg Second-epoch detections are separated by 2.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:49.31 +33:27:50.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.696+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:49.31 +33:27:50.1: 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 22:21:49.31 +33:27:50.1: 14.06 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461179.7895,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.52 21:23:38.46 +35:00:20.4
81.88436 -10.82083 galactic Cyg Second-epoch detections are separated by 6.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:23:38.46 +35:00:20.4 (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 21:23:38.46 +35:00:20.4: 11.94 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:38.46 +35:00:20.4: 13.63 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461179.7895,11.52,0.05,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 20260519.2895 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 19.2895 2461179.7895 11.31 21:52:06.19 +38:25:44.3
88.52650 -12.18146 galactic Cyg Second-epoch detections are separated by 2.7" and 1.0 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 J328.0055+38.4284 | 21:52:03.53 +38:25:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:06.19 +38:25:44.3: 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 21:52:06.19 +38:25:44.3: 13.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J328.0055+38.4284,2461179.7895,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.0055+38.4284 20260519.2895 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.54 21:27:12.66 +39:53:03.7
85.88405 -7.86601 galactic Cyg Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1964684037391843840 | 21:27:10.67 +39:53:34.8 (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 21:27:12.66 +39:53:03.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:12.66 +39:53:03.7: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 1964684037391843840,2461179.7895,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964684037391843840 20260519.2895 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.45 21:49:54.34 +37:45:56.2
87.75036 -12.40922 galactic Cyg Second-epoch detections are separated by 1.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:54.34 +37:45:56.2 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:54.34 +37:45:56.2: 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 21:49:54.34 +37:45:56.2: 14.12 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461179.7895,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.53 21:31:01.72 +37:20:11.1
84.62985 -10.21420 galactic Cyg Second-epoch detections are separated by 1.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952136612550798080 | 21:30:59.63 +37:20:03.4 (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 21:31:01.72 +37:20:11.1: 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 21:31:01.72 +37:20:11.1: 13.28 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 1952136612550798080,2461179.7895,11.53,0.05,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
Gaia DR3 1952136612550798080 20260519.2895 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 19.2895 2461179.7895 10.90 22:24:46.92 +33:34:08.7
90.95317 -20.04189 galactic Peg Second-epoch detections are separated by 1.3" and 1.5 pix
The object was found in VSX 9" Gaia DR3 1902126223810918272
Type: ROT
# Max. Min./Amp. JD0 Period
12.740 G 12.770 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 22:24:46.92 +33:34:08.7: 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 22:24:46.92 +33:34:08.7: 13.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 1902126223810918272,2461179.7895,10.90,0.05,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 1902126223810918272 20260519.2895 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 19.2895 2461179.7895 11.13 22:23:13.49 +34:11:34.8
91.04617 -19.34472 galactic Peg Second-epoch detections are separated by 2.5" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:13.49 +34:11:34.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.398+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:13.49 +34:11:34.8: 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 22:23:13.49 +34:11:34.8: 14.08 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461179.7895,11.13,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.91 22:23:01.57 +32:47:41.3
90.16133 -20.46923 galactic Peg Second-epoch detections are separated by 1.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:01.57 +32:47:41.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:01.57 +32:47:41.3: 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 22:23:01.57 +32:47:41.3: 14.11 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461179.7895,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.09 22:23:52.56 +33:21:51.6
90.66384 -20.10332 galactic Peg Second-epoch detections are separated by 1.7" and 1.8 pix
The object was found in VSX 3" Gaia DR3 1902099560653811072
Type: ROT
# Max. Min./Amp. JD0 Period
13.240 G 13.250 G 0.356109000000 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 22:23:52.56 +33:21:51.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:52.56 +33:21:51.6: 14.28 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.28 +/- 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
Gaia DR3 1902099560653811072,2461179.7895,11.09,0.05,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
Gaia DR3 1902099560653811072 20260519.2895 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 19.2895 2461179.7895 11.57 21:29:41.41 +38:48:31.7
85.47415 -8.97150 galactic Cyg Second-epoch detections are separated by 1.6" and 1.2 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 J322.4223+38.8106 | 21:29:40.43 +38:49:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.686+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:41.41 +38:48:31.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:41.41 +38:48:31.7: 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
ATO J322.4223+38.8106,2461179.7895,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.4223+38.8106 20260519.2895 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.51 21:43:31.94 +38:44:14.3
87.43610 -10.85522 galactic Cyg Second-epoch detections are separated by 0.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 21:43:31.94 +38:44:14.3: 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 21:43:31.94 +38:44:14.3: 13.91 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 1953638957749125248,2461179.7895,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953638957749125248 20260519.2895 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.99 22:24:50.18 +34:08:24.7
91.30590 -19.57695 galactic Peg Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J336.2095+34.1399 | 22:24:50.18 +34:08:24.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M2 (LAMOST DR5) J-Ks=1.123+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:50.18 +34:08:24.7: 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 22:24:50.18 +34:08:24.7: 13.97 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.97 +/- 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
ATO J336.2095+34.1399,2461179.7895,10.99,0.05,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 J336.2095+34.1399 20260519.2895 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 19.2895 2461179.7895 11.45 21:22:48.69 +36:59:06.2
83.19790 -9.31300 galactic Cyg Second-epoch detections are separated by 1.4" and 1.4 pix
The object was found in VSX24" Gaia DR3 1963705231525248512
Type: ROT
# Max. Min./Amp. JD0 Period
12.850 G 12.880 G 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 21:22:48.69 +36:59:06.2: 11.50 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:48.69 +36:59:06.2: 13.51 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 1963705231525248512,2461179.7895,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963705231525248512 20260519.2895 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.07 22:19:31.08 +33:01:21.4
89.66128 -19.85792 galactic Peg Second-epoch detections are separated by 0.4" and 1.6 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 | 22:19:31.08 +33:01:21.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.629+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:31.08 +33:01:21.4: 12.98 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:31.08 +33:01:21.4: 14.33 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461179.7895,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.97 22:23:11.39 +33:56:44.8
90.89074 -19.54394 galactic Peg Second-epoch detections are separated by 2.9" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:11.39 +33:56:44.8 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:11.39 +33:56:44.8: 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 22:23:11.39 +33:56:44.8: 13.99 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461179.7895,10.97,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.02 22:23:44.35 +33:36:35.5
90.78747 -19.88514 galactic Peg Second-epoch detections are separated by 4.0" and 1.6 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 | 22:23:44.35 +33:36:35.5 (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 22:23:44.35 +33:36:35.5: 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 22:23:44.35 +33:36:35.5: 14.13 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461179.7895,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.04 22:23:12.06 +34:06:18.2
90.98887 -19.41426 galactic Peg Second-epoch detections are separated by 1.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:23:12.06 +34:06:18.2 (user input) | T | P | (position from user input) J-Ks=0.777+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:12.06 +34:06:18.2: 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 22:23:12.06 +34:06:18.2: 14.27 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461179.7895,11.04,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.56 21:52:14.84 +36:58:30.1
87.59013 -13.31314 galactic Cyg Second-epoch detections are separated by 1.7" and 1.6 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 | 21:52:14.84 +36:58:30.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.861+/-0.028 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:14.84 +36:58:30.1: 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 21:52:14.84 +36:58:30.1: 14.13 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461179.7895,11.56,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.25 22:24:04.78 +33:37:06.6
90.85474 -19.91830 galactic Peg Second-epoch detections are separated by 1.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:04.78 +33:37:06.6 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:04.78 +33:37:06.6: 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 22:24:04.78 +33:37:06.6: 14.23 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.23 +/- 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,2461179.7895,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.68 21:59:59.99 +38:42:22.6
89.93194 -12.94142 galactic Lac Second-epoch detections are separated by 2.1" and 1.4 pix
The object was found in VSX21" Gaia DR3 1956026134933788544
Type: ROT
# Max. Min./Amp. JD0 Period
18.080 G 18.230 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 21:59:59.99 +38:42:22.6: 13.19 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:59.99 +38:42:22.6: 14.21 +/- 0.11 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
Gaia DR3 1956026134933788544,2461179.7895,11.68,0.05,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
Gaia DR3 1956026134933788544 20260519.2895 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.82 21:14:10.55 +37:06:09.8
82.07624 -7.98880 galactic Cyg Second-epoch detections are separated by 2.0" and 1.2 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 J318.5475+37.1028 | 21:14:10.55 +37:06:09.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.277+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:10.55 +37:06:09.8: 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 21:14:10.55 +37:06:09.8: 14.21 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.21 +/- 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
ATO J318.5475+37.1028,2461179.7895,11.82,0.05,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 J318.5475+37.1028 20260519.2895 11.82CV 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 19.2895 2461179.7895 12.04 21:10:16.65 +40:21:13.7
83.95145 -5.21790 galactic Cyg Second-epoch detections are separated by 3.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.5588+40.3458 | 21:10:16.65 +40:21:13.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:16.65 +40:21:13.7: 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 21:10:16.65 +40:21:13.7: 14.60 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J317.5588+40.3458,2461179.7895,12.04,0.05,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 J317.5588+40.3458 20260519.2895 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.15 22:25:23.93 +34:23:42.5
91.56001 -19.43159 galactic Peg Second-epoch detections are separated by 1.8" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:25:23.93 +34:23:42.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:23.93 +34:23:42.5: 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 22:25:23.93 +34:23:42.5: 13.79 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461179.7895,11.15,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 11.54 22:05:01.78 +41:27:42.7
92.43511 -11.35074 galactic Lac Second-epoch detections are separated by 2.5" and 1.1 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 J331.2733+41.4646 | 22:05:01.78 +41:27:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.327+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:01.78 +41:27:42.7: 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 22:05:01.78 +41:27:42.7: 14.03 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 J331.2733+41.4646,2461179.7895,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2733+41.4646 20260519.2895 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.99 21:16:44.70 +42:11:22.0
86.12877 -4.84156 galactic Cyg Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.2045+42.1963 | 21:16:47.87 +42:11:41.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.572+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:44.70 +42:11:22.0: 13.20 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:44.70 +42:11:22.0: 14.39 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.16 +/- 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
ATO J319.2045+42.1963,2461179.7895,11.99,0.05,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
ATO J319.2045+42.1963 20260519.2895 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 19.2895 2461179.7895 11.69 21:27:03.51 +35:21:31.8
82.64073 -11.06753 galactic Cyg Second-epoch detections are separated by 2.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951313838558088064 | 21:27:06.42 +35:21:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.370+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:03.51 +35:21:31.8: 12.03 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:03.51 +35:21:31.8: 14.09 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 1951313838558088064,2461179.7895,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951313838558088064 20260519.2895 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.80 21:30:44.38 +35:40:19.5
83.40901 -11.36973 galactic Cyg Second-epoch detections are separated by 2.8" and 1.1 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 J322.6833+35.6739 | 21:30:44.38 +35:40:19.5 (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 21:30:44.38 +35:40:19.5: 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 21:30:44.38 +35:40:19.5: 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
ATO J322.6833+35.6739,2461179.7895,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.6833+35.6739 20260519.2895 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.91 21:22:09.19 +38:06:47.4
83.91827 -8.42808 galactic Cyg Second-epoch detections are separated by 1.1" and 1.6 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 | 21:22:09.19 +38:06:47.4 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:09.19 +38:06:47.4: 12.08 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:09.19 +38:06:47.4: 14.26 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.97 +/- 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,2461179.7895,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 12.23 21:12:15.77 +41:54:51.6
85.35342 -4.42836 galactic Cyg Second-epoch detections are separated by 1.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:12:15.77 +41:54:51.6 (user input) | T | P | (position from user input) J-Ks=1.016+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:15.77 +41:54:51.6: 12.57 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:15.77 +41:54:51.6: 14.65 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461179.7895,12.23,0.05,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 20260519.2895 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.50 22:02:41.35 +37:09:20.1
89.37219 -14.48743 galactic Lac Second-epoch detections are separated by 1.0" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:41.35 +37:09:20.1 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:41.35 +37:09:20.1: 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 22:02:41.35 +37:09:20.1: 14.19 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461179.7895,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.96 21:42:10.77 +39:16:10.7
87.59552 -10.28260 galactic Cyg Second-epoch detections are separated by 2.4" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953715648687912064 | 21:42:11.55 +39:16:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.752+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:10.77 +39:16:10.7: 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 21:42:10.77 +39:16:10.7: 14.72 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
Gaia DR3 1953715648687912064,2461179.7895,11.96,0.05,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 1953715648687912064 20260519.2895 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.93 21:44:26.63 +39:22:57.4
88.00520 -10.48785 galactic Cyg Second-epoch detections are separated by 2.1" and 1.2 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 J326.1213+39.3883 | 21:44:26.63 +39:22:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.353+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:26.63 +39:22:57.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:26.63 +39:22:57.4: 14.03 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 J326.1213+39.3883,2461179.7895,11.93,0.05,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
ATO J326.1213+39.3883 20260519.2895 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 19.2895 2461179.7895 12.18 21:48:58.48 +37:54:22.4
87.70083 -12.18290 galactic Cyg Second-epoch detections are separated by 2.0" and 1.6 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 | 21:48:58.48 +37:54:22.4 (user input) | T | P | (position from user input) J-Ks=0.697+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:58.48 +37:54:22.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:58.48 +37:54:22.4: 14.88 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461179.7895,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 12.27 21:42:45.53 +38:41:54.9
87.29501 -10.78409 galactic Cyg Second-epoch detections are separated by 2.3" and 1.0 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 | 21:42:45.53 +38:41:54.9 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:45.53 +38:41:54.9: 12.59 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:45.53 +38:41:54.9: 14.86 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.32 +/- 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,2461179.7895,12.27,0.05,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 20260519.2895 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.82 22:23:06.21 +32:48:02.8
90.17920 -20.47364 galactic Peg Second-epoch detections are separated by 3.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1901976209193816320 | 22:23:06.16 +32:48:05.8 (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 22:23:06.21 +32:48:02.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:06.21 +32:48:02.8: 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 1901976209193816320,2461179.7895,9.82,0.05,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
Gaia DR3 1901976209193816320 20260519.2895 9.82CV 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 19.2895 2461179.7895 10.22 22:24:47.82 +41:23:34.6
95.49853 -13.53780 galactic Lac Second-epoch detections are separated by 1.4" and 1.6 pix
The object was found in VSX13" 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 22:24:47.82 +41:23:34.6: 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 22:24:47.82 +41:23:34.6: 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
Gaia DR3 1957496181979308928,2461179.7895,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1957496181979308928 20260519.2895 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 11.10 22:14:30.42 +34:05:12.7
89.42933 -18.38332 galactic Peg Second-epoch detections are separated by 0.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:14:30.42 +34:05:12.7 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:14:30.42 +34:05:12.7: 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 22:14:30.42 +34:05:12.7: 13.69 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461179.7895,11.10,0.05,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 20260519.2895 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 19.2895 2461179.7895 9.94 22:20:06.30 +33:26:31.1
90.02619 -19.58786 galactic Peg Second-epoch detections are separated by 1.6" and 1.6 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 1905066146106031744 | 22:20:06.38 +33:26:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.721+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:06.30 +33:26:31.1: 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 22:20:06.30 +33:26:31.1: 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
Gaia DR3 1905066146106031744,2461179.7895,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905066146106031744 20260519.2895 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.14 21:52:37.05 +39:29:23.8
89.29902 -11.43055 galactic Cyg Second-epoch detections are separated by 0.3" and 1.4 pix
The object was found in VSX 2" V1736 Cyg
Type: SRA
# Max. Min./Amp. JD0 Period
15.700 B 17.500 B 2443155.00000 289.300000000000
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 21:52:37.05 +39:29:23.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:37.05 +39:29:23.8: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1736 Cyg,2461179.7895,10.14,0.05,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
V1736 Cyg 20260519.2895 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 19.2895 2461179.7895 10.06 22:18:38.88 +33:13:29.2
89.62935 -19.58746 galactic Peg Second-epoch detections are separated by 0.6" and 1.6 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 1905050271906025472 | 22:18:38.97 +33:13:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:38.88 +33:13:29.2: 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 22:18:38.88 +33:13:29.2: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 1905050271906025472,2461179.7895,10.06,0.05,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
Gaia DR3 1905050271906025472 20260519.2895 10.06CV 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 19.2895 2461179.7895 9.19 22:22:47.01 +32:45:45.7
90.09707 -20.46628 galactic Peg Second-epoch detections are separated by 0.7" and 1.6 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 1901981947270002560 | 22:22:47.18 +32:45:44.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.315+/-0.024 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:47.01 +32:45:45.7: 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 22:22:47.01 +32:45:45.7: 12.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1901981947270002560,2461179.7895,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1901981947270002560 20260519.2895 9.19CV 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 19.2895 2461179.7895 10.39 22:19:16.62 +33:14:56.7
89.75782 -19.64442 galactic Peg Second-epoch detections are separated by 2.2" and 1.6 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 1905039551667803776 | 22:19:16.65 +33:14:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.581+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:16.62 +33:14:56.7: 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 22:19:16.62 +33:14:56.7: 13.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 1905039551667803776,2461179.7895,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1905039551667803776 20260519.2895 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.61 22:26:22.08 +38:29:11.0
94.11372 -16.13532 galactic Lac Second-epoch detections are separated by 0.5" and 1.6 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 1908614407566589056 | 22:26:22.17 +38:29:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:22.08 +38:29:11.0: 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 22:26:22.08 +38:29:11.0: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 1908614407566589056,2461179.7895,9.61,0.05,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 1908614407566589056 20260519.2895 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 19.2895 2461179.7895 9.53 22:27:04.56 +36:34:03.6
93.13430 -17.81573 galactic Lac Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1907557914331273856 | 22:27:04.63 +36:34:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.204+/-0.029 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:04.56 +36:34:03.6: 13.30 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:04.56 +36:34:03.6: 12.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 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 1907557914331273856,2461179.7895,9.53,0.05,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
Gaia DR3 1907557914331273856 20260519.2895 9.53CV 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 19.2895 2461179.7895 9.93 22:25:31.35 +36:37:30.5
92.89492 -17.59545 galactic Lac Second-epoch detections are separated by 0.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1906074703207024128 | 22:25:31.39 +36:37:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.080+/-0.028 (A)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:31.35 +36:37:30.5: 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 22:25:31.35 +36:37:30.5: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 1906074703207024128,2461179.7895,9.93,0.05,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 1906074703207024128 20260519.2895 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 19.2895 2461179.7895 10.04 22:26:48.56 +40:52:45.3
95.53810 -14.17496 galactic Lac Second-epoch detections are separated by 1.3" and 1.6 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 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 22:26:48.56 +40:52:45.3: 13.10 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:48.56 +40:52:45.3: 12.94 +/- 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 1909383172354020096,2461179.7895,10.04,0.05,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
Gaia DR3 1909383172354020096 20260519.2895 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 19.2895 2461179.7895 10.05 22:28:59.62 +41:10:52.3
96.06376 -14.14207 galactic Lac Second-epoch detections are separated by 0.5" and 1.5 pix
The object was found in VSX 1" ASASSN-V J222859.65+411053.3
Type: EA
# Max. Min./Amp. JD0 Period
12.360 V 12.940 V 2457223.04300 2.456890000000
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 22:28:59.62 +41:10:52.3: 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 22:28:59.62 +41:10:52.3: 13.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.00 +/- 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
ASASSN-V J222859.65+411053.3,2461179.7895,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J222859.65+411053.3 20260519.2895 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.90 22:26:09.53 +39:20:23.0
94.56373 -15.39892 galactic Lac Second-epoch detections are separated by 0.8" and 1.5 pix
The object was found in VSX 1" Gaia DR3 1908862106921553792
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.980 G 12.100 G 0.086366100000 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 22:26:09.53 +39:20:23.0: 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 22:26:09.53 +39:20:23.0: 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
Gaia DR3 1908862106921553792,2461179.7895,9.90,0.05,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 1908862106921553792 20260519.2895 9.90CV 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 19.2895 2461179.7895 8.55 22:23:22.75 +33:27:23.4
90.62899 -19.96851 galactic Peg Second-epoch detections are separated by 1.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1902150859743177984 | 22:23:22.68 +33:27:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.192+/-0.025 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:22.75 +33:27:23.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:22.75 +33:27:23.4: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1902150859743177984,2461179.7895,8.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1902150859743177984 20260519.2895 8.55CV 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 19.2895 2461179.7895 10.20 22:27:58.20 +41:56:15.7
96.31410 -13.40055 galactic Lac Second-epoch detections are separated by 1.4" and 1.6 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 1957578649651122944 | 22:27:58.25 +41:56:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:58.20 +41:56:15.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:58.20 +41:56:15.7: 13.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 1957578649651122944,2461179.7895,10.20,0.05,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
Gaia DR3 1957578649651122944 20260519.2895 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.63 22:26:35.14 +36:30:44.8
93.01602 -17.80748 galactic Lac Second-epoch detections are separated by 0.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1906059245621689088 | 22:26:35.23 +36:30:45.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.216+/-0.034 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:35.14 +36:30:44.8: 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 22:26:35.14 +36:30:44.8: 12.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1906059245621689088,2461179.7895,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1906059245621689088 20260519.2895 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.03 22:28:14.10 +38:59:33.1
94.71822 -15.90917 galactic Lac Second-epoch detections are separated by 1.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1908657696539857920 | 22:28:14.12 +38:59:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:14.10 +38:59:33.1: 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 22:28:14.10 +38:59:33.1: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 1908657696539857920,2461179.7895,10.03,0.05,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 1908657696539857920 20260519.2895 10.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 9.59 22:27:40.80 +38:24:06.8
94.28978 -16.34642 galactic Lac Second-epoch detections are separated by 0.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1908557885797202176 | 22:27:40.87 +38:24:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.180+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:40.80 +38:24:06.8: 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 22:27:40.80 +38:24:06.8: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1908557885797202176,2461179.7895,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1908557885797202176 20260519.2895 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.46 22:24:04.58 +41:44:25.4
95.57803 -13.17324 galactic Lac Second-epoch detections are separated by 0.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:24:04.58 +41:44:25.4 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:04.58 +41:44:25.4: 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 22:24:04.58 +41:44:25.4: 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,2461179.7895,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.45 22:15:55.09 +33:10:18.4
89.10647 -19.29452 galactic Peg Second-epoch detections are separated by 0.2" and 1.5 pix
The object was found in VSX11" Gaia DR3 1899102876073302528
Type: ROT
# Max. Min./Amp. JD0 Period
15.480 G 15.510 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 22:15:55.09 +33:10:18.4: 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 22:15:55.09 +33:10:18.4: 13.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 1899102876073302528,2461179.7895,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1899102876073302528 20260519.2895 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.51 22:24:41.58 +41:00:04.8
95.26116 -13.85490 galactic Lac Second-epoch detections are separated by 1.0" and 1.6 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 J336.1583+41.0030 | 22:24:41.58 +41:00:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:41.58 +41:00:04.8: 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 22:24:41.58 +41:00:04.8: 13.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 J336.1583+41.0030,2461179.7895,10.51,0.05,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 20260519.2895 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 19.2895 2461179.7895 10.62 22:20:34.56 +41:55:58.2
95.12992 -12.65234 galactic Lac Second-epoch detections are separated by 0.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.1491+41.9350 | 22:20:34.56 +41:55:58.2 (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 22:20:34.56 +41:55:58.2: 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 22:20:34.56 +41:55:58.2: 13.53 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 J335.1491+41.9350,2461179.7895,10.62,0.05,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 J335.1491+41.9350 20260519.2895 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 19.2895 2461179.7895 10.72 22:27:32.21 +40:12:34.8
95.28387 -14.81281 galactic Lac Second-epoch detections are separated by 0.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:32.21 +40:12:34.8 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:32.21 +40:12:34.8: 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 22:27:32.21 +40:12:34.8: 13.65 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461179.7895,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.56 22:21:24.84 +40:44:14.8
94.57903 -13.73217 galactic Lac Second-epoch detections are separated by 0.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:24.84 +40:44:14.8 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:24.84 +40:44:14.8: 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 22:21:24.84 +40:44:14.8: 13.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 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,2461179.7895,10.56,0.05,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
target 20260519.2895 10.56CV 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 19.2895 2461179.7895 11.24 21:59:24.47 +39:22:40.2
90.26722 -12.34378 galactic Lac Second-epoch detections are separated by 2.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:24.47 +39:22:40.2 (user input) | T | P | (position from user input) J-Ks=1.648+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:24.47 +39:22:40.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:24.47 +39:22:40.2: 14.04 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461179.7895,11.24,0.05,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
target 20260519.2895 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 19.2895 2461179.7895 10.53 22:18:40.15 +33:30:22.2
89.80737 -19.36156 galactic Peg Second-epoch detections are separated by 0.4" and 1.6 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 | 22:18:40.15 +33:30:22.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.658+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:40.15 +33:30:22.2: 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 22:18:40.15 +33:30:22.2: 13.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.44 +/- 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,2461179.7895,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260519.2895 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 19.2895 2461179.7895 10.44 22:18:38.97 +33:24:05.6
89.73913 -19.44413 galactic Peg Second-epoch detections are separated by 4.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:38.97 +33:24:05.6 (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 22:18:38.97 +33:24:05.6: 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 22:18:38.97 +33:24:05.6: 13.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461179.7895,10.44,0.05,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 20260519.2895 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
## 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: 2461179.78965866 19.05.2026 06:56:56.508 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 76
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: 7 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): 21675
Objects passed selection criteria: 21662
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 20635.8
Average stars matched: 20283 (98.2906 %)
Memory usage VmPeak: 127836 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon May 18 15:05:05 CDT 2026
VaST build number 1.0rc89-60-gf8f75ec6
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-18)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 19 02:29:16 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: 2461179.78965866 19.05.2026 06:56:56.508 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 751
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: 83 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): 133219
Objects passed selection criteria: 133080
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: 137153
Average stars matched: 134852 (98.3223 %)
Memory usage VmPeak: 1939456 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon May 18 15:05:05 CDT 2026
VaST build number 1.0rc89-60-gf8f75ec6
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-18)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 19 02:32:45 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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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: 2461179.78924895
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_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits'
wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
Image size: 942.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:49:05.784 +38:00:12.31 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 21:49:05.784 +38:00:12.31
Angular distance between the image centers 0.0418 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
Image size: 942.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:49:06.460 +38:00:15.54 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 21:49:06.460 +38:00:15.54
Angular distance between the image centers 0.0425 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 21:49:05.784 +38:00:12.31
Second-epoch second image center 21:49:06.460 +38:00:15.54
Angular distance between the image centers 0.00239 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.DqJ4jSXAF5
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.pWcPSTDwzu
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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits &> /tmp/tmp.e6T22T1rcd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits &> /tmp/tmp.WL8PoS9xZo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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 60 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
2.5 pix fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
2.5 pix fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
14.5 mag. fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DqJ4jSXAF5 (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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/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.pWcPSTDwzu (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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/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.e6T22T1rcd (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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
Checking if the catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.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_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
WCS catalog name: wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=901, passed=16414
Got 16414 stars (including 15496 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat
util/solve_plate_with_UCAC5 got 16414 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits N_match=953 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.496 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.355 n_q1=270 n_q2=140 n_q3=352 n_q4=191 worst_quadrant_to_overall_ratio=1.381
The image catalog is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits -region wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.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.WL8PoS9xZo (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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
Checking if the catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat corresponding to the image wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
WCS catalog name: wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=920, passed=16457
Got 16457 stars (including 15518 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat
util/solve_plate_with_UCAC5 got 16457 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (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: 952 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 16059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (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: 952 matched stars entering correct_measured_positions(), 16061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 16060 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits N_match=952 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.446 sigma_q2_arcsec=0.439 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.413 n_q1=265 n_q2=145 n_q3=348 n_q4=194 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits -region wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits sigma_overall=0.359 worst_q_ratio=1.381
new2=fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits sigma_overall=0.369 worst_q_ratio=1.210
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_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286_astrometric_residuals.png (953 matched stars from wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287_astrometric_residuals.png (952 matched stars from wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-21_20.00sec_-0.00C_LIGHTs_0286.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Cyg-07-Q1b1x1_022650_TTUQ1b1x1_2233052_OTTS8N1m/wcs_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287.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 22:19:05.16 +32:54:15.2: 15.15 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:38.63 +33:28:07.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:02.85 +32:44:45.5: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:51.01 +32:30:49.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:22.33 +32:32:02.8: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:42.78 +32:35:19.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:54.19 +32:28:51.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:13.33 +32:50:51.8: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:28.75 +32:41:44.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:22.33 +32:32:02.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:21:22.33 +32:32:02.8: 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 22:23:42.78 +32:35:19.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:23:42.78 +32:35:19.8: 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 22:20:51.01 +32:30:49.7: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:20:51.01 +32:30:49.7: 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 22:20:54.19 +32:28:51.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:20:54.19 +32:28:51.0: 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 22:21:28.75 +32:41:44.1: 10.61 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:05.16 +32:54:15.2: 9.95 +/- 0.00 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:38.63 +33:28:07.3: 9.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.61 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:28.75 +32:41:44.1: ref_mag=10.61 +/- 0.01 new_mean_mag=10.2725 delta=0.34 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:13.33 +32:50:51.8: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.77 +/- 0.00
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:02.85 +32:44:45.5: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.95 +/- 0.00
Forced photometry filter REJECTED candidate at 22:22:38.63 +33:28:07.3: ref_mag=9.77 +/- 0.00 new_mean_mag=9.4870 delta=0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:19:05.16 +32:54:15.2: ref_mag=9.95 +/- 0.00 new_mean_mag=9.7671 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter REJECTED candidate at 22:22:13.33 +32:50:51.8: ref_mag=10.38 +/- 0.00 new_mean_mag=10.0815 delta=0.30 (need > 0.90)
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter REJECTED candidate at 22:22:02.85 +32:44:45.5: ref_mag=10.23 +/- 0.00 new_mean_mag=9.9009 delta=0.33 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:54.66 +33:02:51.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:08.17 +32:26:31.3: 13.71 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:08.17 +32:26:31.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:24:08.17 +32:26:31.3: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:29.71 +32:27:27.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:12.31 +32:53:20.1: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:29.71 +32:27:27.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:23:29.71 +32:27:27.3: 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 22:23:54.66 +33:02:51.1: 10.70 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:19.15 +32:44:18.4: 15.68 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.70 +/- 0.01
Forced photometry filter REJECTED candidate at 22:23:54.66 +33:02:51.1: ref_mag=10.70 +/- 0.01 new_mean_mag=10.3881 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 22:23:40.83 +32:17:33.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:38.63 +32:18:22.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:40.83 +32:17:33.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:23:40.83 +32:17:33.4: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:01.21 +32:38:34.6: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:38.63 +32:18:22.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:20:38.63 +32:18:22.4: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:34.15 +32:37:28.5: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:12.31 +32:53:20.1: 10.82 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:01.21 +32:38:34.6: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:18:01.21 +32:38:34.6: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 10.82 +/- 0.01
Forced photometry filter REJECTED candidate at 22:24:12.31 +32:53:20.1: ref_mag=10.82 +/- 0.01 new_mean_mag=10.5496 delta=0.27 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:34.15 +32:37:28.5: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:19:34.15 +32:37:28.5: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:09.16 +32:29:58.8: 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 22:19:19.15 +32:44:18.4: 11.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.01
Forced photometry filter REJECTED candidate at 22:19:19.15 +32:44:18.4: ref_mag=11.01 +/- 0.01 new_mean_mag=10.7157 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 22:23:09.16 +32:29:58.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:23:09.16 +32:29:58.8: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:19.10 +32:17:17.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:45.77 +32:38:27.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:19.10 +32:17:17.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:19:19.10 +32:17:17.3: 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 22:18:45.77 +32:38:27.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:18:45.77 +32:38:27.0: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:13.07 +32:41:36.2: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:07.69 +32:21:25.5: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:07.69 +32:21:25.5: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:24:07.69 +32:21:25.5: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:06.58 +32:34:23.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:09.24 +32:52:45.4: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:06.58 +32:34:23.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:22:06.58 +32:34:23.8: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:18.83 +32:47:18.5: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:43.92 +33:23:34.8: 13.84 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:13.07 +32:41:36.2: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:20.23 +32:26:10.0: 15.68 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:22:13.07 +32:41:36.2: ref_mag=11.20 +/- 0.01 new_mean_mag=10.9497 delta=0.25 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:35.29 +32:31:15.8: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:20.23 +32:26:10.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:20:20.23 +32:26:10.0: 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 22:23:35.29 +32:31:15.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:23:35.29 +32:31:15.8: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:23.77 +32:48:56.5: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:02.70 +32:39:05.4: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:09.24 +32:52:45.4: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:09.24 +32:52:45.4: ref_mag=11.36 +/- 0.01 new_mean_mag=11.0952 delta=0.27 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:07.15 +32:50:48.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:18.83 +32:47:18.5: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:18.83 +32:47:18.5: ref_mag=11.27 +/- 0.01 new_mean_mag=11.0853 delta=0.19 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:24.83 +32:18:11.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:43.92 +33:23:34.8: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry filter REJECTED candidate at 22:23:43.92 +33:23:34.8: ref_mag=11.55 +/- 0.01 new_mean_mag=11.1255 delta=0.43 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:24.83 +32:18:11.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:19:24.83 +32:18:11.9: 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 22:24:02.70 +32:39:05.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:24:02.70 +32:39:05.4: 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 22:22:23.77 +32:48:56.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
Forced photometry filter REJECTED candidate at 22:22:23.77 +32:48:56.5: ref_mag=11.36 +/- 0.01 new_mean_mag=11.1278 delta=0.23 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:29.19 +32:18:20.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:07.15 +32:50:48.8: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:29.19 +32:18:20.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:22:29.19 +32:18:20.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry filter REJECTED candidate at 22:20:07.15 +32:50:48.8: ref_mag=11.41 +/- 0.01 new_mean_mag=11.1514 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:30.36 +32:41:34.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:09.09 +32:25:23.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:09.09 +32:25:23.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:18:09.09 +32:25:23.0: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:12.47 +33:23:25.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:19.57 +39:36:36.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:11.62 +32:43:33.3: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:20.59 +32:49:59.1: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:30.36 +32:41:34.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:20:30.36 +32:41:34.9: 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_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:47.51 +32:45:41.6: 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 22:18:46.80 +32:43:54.9: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:42.86 +32:57:56.1: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:11.62 +32:43:33.3: 11.81 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:19.57 +39:36:36.8: 11.14 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:12.47 +33:23:25.7: 11.79 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:20.59 +32:49:59.1: 11.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.02
Forced photometry reference-image weighted average: 11.14 +/- 0.01
Forced photometry reference-image weighted average: 11.79 +/- 0.02
Forced photometry filter REJECTED candidate at 22:18:11.62 +32:43:33.3: ref_mag=11.81 +/- 0.02 new_mean_mag=11.5041 delta=0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:49:19.57 +39:36:36.8: ref_mag=11.14 +/- 0.01 new_mean_mag=11.7668 delta=-0.63 (need > 0.90)
Forced photometry reference-image weighted average: 11.78 +/- 0.02
Forced photometry filter REJECTED candidate at 22:23:12.47 +33:23:25.7: ref_mag=11.79 +/- 0.02 new_mean_mag=11.4470 delta=0.34 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:24:20.59 +32:49:59.1: ref_mag=11.78 +/- 0.02 new_mean_mag=11.5068 delta=0.28 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:41.98 +42:12:29.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:47.51 +32:45:41.6: 12.03 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:46.80 +32:43:54.9: 11.97 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:42.86 +32:57:56.1: 11.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.02
Forced photometry filter REJECTED candidate at 22:22:47.51 +32:45:41.6: ref_mag=12.03 +/- 0.02 new_mean_mag=11.6496 delta=0.38 (need > 0.90)
Forced photometry reference-image weighted average: 11.97 +/- 0.02
Forced photometry reference-image weighted average: 11.89 +/- 0.02
Forced photometry filter REJECTED candidate at 22:21:42.86 +32:57:56.1: ref_mag=11.89 +/- 0.02 new_mean_mag=11.6445 delta=0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:18:46.80 +32:43:54.9: ref_mag=11.97 +/- 0.02 new_mean_mag=11.7603 delta=0.21 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:22.74 +33:27:24.2: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:41.98 +42:12:29.0: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.01
Forced photometry filter REJECTED candidate at 22:27:41.98 +42:12:29.0: ref_mag=11.10 +/- 0.01 new_mean_mag=10.7468 delta=0.35 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:22.74 +33:27:24.2: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Forced photometry filter REJECTED candidate at 22:23:22.74 +33:27:24.2: ref_mag=11.27 +/- 0.01 new_mean_mag=11.0057 delta=0.26 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 31064_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31064_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31071_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31071_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31082_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31082_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31085_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31085_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:20:59.13 +33:19:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31093_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31093_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31099_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31099_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31102_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31102_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31104_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31104_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31109_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31109_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31115_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31115_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31131_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31131_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:38.50 +33:27:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31132_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31132_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31133_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31133_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31134_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31134_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:29.52 +33:00:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31146_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31146_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31156_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31156_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31167_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31167_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31175_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31175_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31176_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31176_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31194_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31194_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31197_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31197_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:20:14.11 +32:57:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31198_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31198_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31201_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31201_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:50.27 +33:30:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31203_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31203_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31206_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31206_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31211_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31211_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31213_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31213_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31214_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31214_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:22:45.69 +32:58:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31220_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31220_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:31.00 +33:12:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31225_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31225_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31232_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31232_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31237_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31237_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31238_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31238_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31240_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31240_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31242_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31242_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31244_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31244_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31255_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31255_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31257_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31257_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31260_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31260_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31261_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31261_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:37.65 +33:14:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31273_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31273_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:47.54 +33:40:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31276_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31276_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:25:01.22 +33:41:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31281_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31281_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31284_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31284_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31292_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31292_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:12.73 +33:56:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31301_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31301_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31304_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31304_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31324_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31324_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31326_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31326_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31328_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31328_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31338_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31338_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:29.88 +34:04:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31340_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31340_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31351_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31351_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:55.20 +33:13:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31360_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31360_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:22:50.79 +33:41:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31364_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31364_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31372_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31372_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 31376_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 31376_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 30039_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 30039_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 30130_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 30130_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:26:25.61 +37:06:14.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 25413_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 25413_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218161_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218161_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218162_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218162_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218164_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218164_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218166_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218166_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218170_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218170_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218176_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218176_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218177_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218177_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218185_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218185_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:13:42.50 +38:37:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218190_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218190_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218191_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218191_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218196_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218196_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218197_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218197_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218199_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218199_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218200_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218200_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218204_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218204_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218207_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218207_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218211_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218211_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:20:54.56 +38:29:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218213_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218213_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218216_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218216_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218217_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218217_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218220_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218220_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218222_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218222_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218227_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218227_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218228_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218228_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218232_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218232_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218234_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218234_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218236_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218236_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218240_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218240_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218242_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218242_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218243_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218243_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218244_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218244_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218247_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218247_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218249_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218249_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218250_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218250_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218254_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218254_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:12:53.54 +42:27:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218256_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218256_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218257_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218257_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218260_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218260_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218263_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218263_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218265_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218265_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218266_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218266_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:20:04.79 +38:54:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218267_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218267_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218268_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218268_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218269_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218269_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:14:47.01 +43:09:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218272_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218272_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:17:17.34 +34:20:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218273_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218273_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218274_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218274_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218275_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218275_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218281_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218281_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:22:50.01 +33:35:44.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 218283_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218283_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:18:28.74 +32:46:33.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 218290_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218290_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:22:51.01 +33:43:03.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 218299_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218299_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:18:00.93 +32:58:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218309_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218309_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218314_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218314_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218317_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218317_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218318_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218318_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:20:26.96 +33:32:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218331_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218331_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218334_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218334_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:20:59.11 +33:19:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218340_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218340_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218350_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218350_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:18:54.19 +33:04:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218351_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218351_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218353_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218353_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218354_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218354_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218356_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218356_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218361_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218361_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218363_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218363_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218370_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218370_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218384_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218384_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:54.17 +34:03:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218385_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218385_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:38.51 +33:27:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218387_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218387_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218389_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218389_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:29.48 +33:00:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218390_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218390_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:31.06 +33:54:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218391_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218391_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218402_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218402_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:20:50.91 +33:27:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218403_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218403_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 218405_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218405_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218412_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218412_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218426_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218426_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218438_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218438_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218453_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218453_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218457_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218457_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:50.27 +33:30:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218458_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218458_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218459_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218459_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:20:14.07 +32:57:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218461_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218461_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218465_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218465_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218472_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218472_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218474_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218474_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218475_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218475_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:23.37 +34:13:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218476_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218476_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 218477_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218477_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:22:18.61 +33:48:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218487_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218487_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218491_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218491_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218495_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218495_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218499_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218499_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218503_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218503_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218504_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218504_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218512_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218512_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218513_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218513_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:53.85 +34:06:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218518_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218518_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218520_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218520_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218533_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218533_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:37.60 +33:14:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218538_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218538_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218544_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218544_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218547_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218547_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218550_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218550_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:24:12.67 +33:56:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218556_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218556_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:16.05 +33:07:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218563_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218563_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218566_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218566_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218578_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218578_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 218581_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218581_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218588_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218588_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218591_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218591_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218598_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218598_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 218608_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218608_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:14:25.88 +34:53:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218609_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218609_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218615_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218615_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:55.19 +33:13:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218619_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218619_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218631_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218631_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:22:50.75 +33:41:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218632_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218632_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218637_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218637_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218644_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218644_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218645_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218645_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218647_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218647_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:19:38.40 +33:06:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218652_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218652_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218655_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218655_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218659_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218659_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218667_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218667_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218671_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218671_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218672_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218672_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218674_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218674_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218682_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218682_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 218686_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218686_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218699_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218699_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218702_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218702_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218709_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218709_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218718_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218718_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218722_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218722_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218733_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218733_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218735_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218735_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218736_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218736_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218737_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218737_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218739_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218739_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218740_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218740_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218742_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218742_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218750_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218750_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218753_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218753_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218760_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218760_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218761_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218761_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218769_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218769_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:17:35.89 +39:23:57.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218770_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218770_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218774_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218774_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218775_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218775_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218778_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218778_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218787_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218787_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:22.16 +42:04:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218796_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218796_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218805_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218805_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218806_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218806_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218811_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218811_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218816_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218816_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218820_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218820_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218834_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218834_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218836_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218836_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218837_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218837_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:47:14.34 +41:48:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218842_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218842_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218847_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218847_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:19:43.24 +41:56:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218859_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218859_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218860_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218860_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218861_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218861_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218862_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218862_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218869_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218869_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218871_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218871_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:09:40.80 +42:24:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218873_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218873_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218874_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218874_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218905_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218905_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218906_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218906_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218907_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218907_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218909_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218909_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:19:01.94 +41:01:26.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218916_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218916_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218917_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218917_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218921_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218921_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218923_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218923_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218924_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218924_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218925_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218925_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218930_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218930_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218935_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218935_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218939_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218939_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218940_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218940_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218942_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218942_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218943_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218943_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218944_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218944_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218945_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218945_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218946_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218946_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218956_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218956_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218972_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218972_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 218978_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218978_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:12:19.83 +40:08:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218987_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218987_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:13:15.17 +35:20:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218992_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218992_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218994_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218994_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218995_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 218995_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 218996_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 218996_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219002_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219002_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219010_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219010_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219019_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219019_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219029_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219029_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219031_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219031_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219033_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219033_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219034_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219034_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219035_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219035_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:13:19.10 +35:28:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219036_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219036_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219037_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219037_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219038_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219038_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219040_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219040_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219044_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219044_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219053_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219053_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219054_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219054_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219058_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219058_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219060_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219060_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219062_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219062_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219063_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219063_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219065_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219065_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 219068_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219068_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:12:55.61 +35:49:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219069_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219069_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219075_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219075_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219076_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219076_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219082_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219082_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219086_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219086_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219087_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219087_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219088_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219088_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219092_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219092_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219097_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219097_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219118_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219118_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219119_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219119_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219120_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219120_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219122_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219122_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219125_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219125_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219132_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219132_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219140_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219140_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219148_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219148_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219152_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219152_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219156_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219156_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219159_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219159_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219169_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219169_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219171_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219171_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219172_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219172_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219177_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219177_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219183_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219183_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:11:41.11 +38:09:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219184_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219184_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219187_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219187_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219198_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219198_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219204_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219204_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:11:02.01 +38:21:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219205_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219205_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219210_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219210_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219213_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219213_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219215_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219215_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219216_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219216_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219219_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219219_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219222_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219222_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219223_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219223_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219233_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219233_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219234_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219234_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219236_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219236_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219237_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219237_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219238_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219238_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219245_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219245_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219250_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219250_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219255_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219255_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219256_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219256_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219257_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219257_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219260_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219260_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219264_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219264_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219271_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219271_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219272_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219272_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219273_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219273_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219274_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219274_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219275_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219275_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219280_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219280_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219287_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219287_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219290_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219290_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219291_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219291_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219293_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219293_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219297_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219297_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219300_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219300_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219303_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219303_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219305_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219305_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:14:53.17 +38:04:34.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 219306_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219306_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219308_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219308_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219312_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219312_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219313_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219313_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219314_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219314_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219315_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219315_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 219316_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219316_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219317_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219317_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219322_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219322_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219325_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219325_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219331_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219331_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219334_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219334_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219335_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219335_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219336_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219336_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219342_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219342_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219343_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219343_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219344_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219344_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:24:49.84 +34:10:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219345_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219345_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219348_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219348_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219349_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219349_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219350_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219350_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:19:30.00 +37:15:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219359_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219359_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219364_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219364_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219372_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219372_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219373_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219373_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219374_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219374_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219377_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219377_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219379_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219379_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219381_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219381_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219382_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219382_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219399_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219399_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219400_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219400_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219401_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219401_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219405_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219405_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219406_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219406_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:15:58.42 +38:39:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219407_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219407_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219408_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219408_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:14:27.18 +38:46:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219412_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219412_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219413_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219413_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219416_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219416_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219423_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219423_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219424_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219424_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219425_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219425_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219427_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219427_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219431_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219431_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219436_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219436_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 219442_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219442_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:16:33.01 +37:16:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219443_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219443_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:10:56.02 +35:44:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219445_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219445_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:13:11.45 +36:44:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219447_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219447_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219448_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219448_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219455_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219455_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219456_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219456_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219457_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219457_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219465_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219465_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219472_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219472_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219474_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219474_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219475_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219475_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219476_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219476_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219477_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219477_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219479_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219479_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219482_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219482_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219483_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219483_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219485_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219485_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:09:38.20 +40:37:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219486_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219486_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219489_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219489_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219490_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219490_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219492_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219492_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219493_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219493_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219495_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219495_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219496_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219496_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219497_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219497_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219498_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219498_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219501_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219501_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219503_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219503_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219507_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219507_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219508_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219508_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219509_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219509_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219511_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219511_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219516_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219516_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219517_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219517_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219529_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219529_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219531_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219531_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219532_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219532_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219537_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219537_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:41:07.23 +41:16:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219542_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219542_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219543_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219543_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219548_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219548_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:31:08.77 +43:06:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219553_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219553_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219554_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219554_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219557_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219557_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219559_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219559_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219562_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219562_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219563_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219563_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219564_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219564_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219568_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219568_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219573_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219573_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219574_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219574_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219578_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219578_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219579_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219579_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219582_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219582_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219583_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219583_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219584_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219584_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219598_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219598_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219601_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219601_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219605_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219605_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219610_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219610_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219612_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219612_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219617_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219617_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219622_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219622_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219624_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219624_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219626_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219626_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219631_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219631_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219643_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219643_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219646_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219646_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219647_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219647_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219653_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219653_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219654_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219654_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219657_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219657_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219665_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219665_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219670_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219670_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219675_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219675_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219677_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219677_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219680_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219680_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219682_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219682_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219689_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219689_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219695_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219695_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219701_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219701_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:49:15.93 +43:03:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219704_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219704_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219715_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219715_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:15:30.14 +37:18:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219717_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219717_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219723_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219723_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219727_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219727_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219729_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219729_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219731_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219731_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219732_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219732_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219734_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219734_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219740_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219740_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219742_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219742_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219743_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219743_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219747_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219747_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219748_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219748_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219752_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219752_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219755_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219755_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219756_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219756_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219757_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219757_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219759_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219759_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:10:53.92 +34:42:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219765_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219765_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219769_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219769_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219771_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219771_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219772_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219772_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219777_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219777_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219789_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219789_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219791_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219791_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219792_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219792_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219793_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219793_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219797_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219797_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219800_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219800_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219802_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219802_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219805_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219805_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219808_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219808_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219810_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219810_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:19:57.44 +43:06:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219812_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219812_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219814_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219814_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219815_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219815_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219818_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219818_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:15:01.85 +41:23:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219819_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219819_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219822_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219822_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219823_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219823_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219826_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219826_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219827_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219827_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219833_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219833_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219836_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219836_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219837_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219837_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219838_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219838_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219840_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219840_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:16:46.54 +43:11:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219841_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219841_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219842_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219842_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219844_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219844_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219846_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219846_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219848_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219848_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219849_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219849_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219850_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219850_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219851_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219851_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219853_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219853_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219858_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219858_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219859_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219859_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219862_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219862_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219873_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219873_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219875_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219875_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219891_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219891_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219892_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219892_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219898_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219898_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219900_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219900_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219908_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219908_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219909_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219909_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219911_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219911_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219913_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219913_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219917_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219917_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219921_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219921_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219925_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219925_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219926_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219926_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219935_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219935_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219943_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219943_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219949_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219949_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219959_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219959_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219964_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219964_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219965_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219965_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219972_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219972_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219973_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219973_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219974_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219974_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219976_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219976_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:32:47.22 +41:31:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219977_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219977_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219980_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219980_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219985_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219985_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219991_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219991_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 219992_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 219992_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 219997_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 219997_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220003_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220003_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220005_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220005_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:42.46 +33:18:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220006_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220006_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220007_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220007_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220010_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220010_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220015_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220015_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220024_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220024_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220028_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220028_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220029_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220029_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220035_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220035_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220036_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220036_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220038_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220038_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220050_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220050_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220054_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220054_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220059_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220059_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220060_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220060_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220069_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220069_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220071_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220071_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220080_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220080_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220081_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220081_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:48:38.36 +41:48:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220082_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220082_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220086_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220086_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220089_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220089_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220090_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220090_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220091_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220091_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220096_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220096_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220101_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220101_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220102_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220102_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220104_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220104_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220114_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220114_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220122_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220122_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220123_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220123_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220125_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220125_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220129_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220129_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220130_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220130_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220135_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220135_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220137_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220137_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220140_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220140_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220147_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220147_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220148_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220148_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220149_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220149_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220151_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220151_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220152_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220152_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220159_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220159_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220161_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220161_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220165_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220165_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220171_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220171_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220177_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220177_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220193_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220193_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220199_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220199_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220203_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220203_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220204_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220204_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220205_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220205_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220211_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220211_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220212_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220212_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220214_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220214_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220216_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220216_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220228_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220228_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220229_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220229_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220230_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220230_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220232_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220232_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220236_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220236_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220237_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220237_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220239_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220239_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220244_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220244_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220253_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220253_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220264_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220264_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220270_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220270_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220285_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220285_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220295_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220295_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220297_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220297_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220307_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220307_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220309_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220309_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220311_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220311_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220343_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220343_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220353_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220353_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220362_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220362_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220364_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220364_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220365_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220365_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220368_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220368_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 220379_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220379_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220380_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220380_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220383_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220383_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220389_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220389_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220391_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220391_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220397_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220397_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220399_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220399_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220403_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220403_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220404_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220404_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220407_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220407_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220413_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220413_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220428_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220428_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220438_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220438_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220441_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220441_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220449_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220449_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220450_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220450_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 220468_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220468_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220498_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220498_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220502_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220502_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220506_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220506_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220507_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220507_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220515_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220515_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220520_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220520_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220529_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220529_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220548_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220548_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220549_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220549_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220554_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220554_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220560_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 220560_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 220572_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220572_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220577_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220577_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220587_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220587_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220601_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220601_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220619_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220619_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220622_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220622_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220652_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220652_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220690_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220690_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 220695_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 220695_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 159333_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 159333_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212246_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212246_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 153315_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 153315_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 213536_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 213536_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:25:55.49 +37:02:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213698_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 213698_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:50.18 +33:55:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147051_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 147051_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:25:27.21 +35:23:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177673_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 177673_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 187418_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 187418_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:40.85 +34:26:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168876_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 168876_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 75482_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 75482_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 164563_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 164563_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 33331_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 33331_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:26:52.25 +41:39:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197094_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 197094_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 158649_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 158649_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 121426_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 121426_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 213696_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 213696_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:23:13.81 +34:27:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42459_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 42459_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 21:18:30.79 +41:07:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213286_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 213286_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:21:48.52 +36:37:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165617_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 165617_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 213146_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 213146_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212977_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212977_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212926_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212926_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212847_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212847_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212846_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212846_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212836_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212836_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 170281_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 170281_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212784_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212784_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212767_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212767_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212711_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212711_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212533_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212533_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212489_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212489_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 163016_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 163016_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212353_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212353_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212306_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212306_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212282_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 212282_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
**** FOUND 22:16:19.05 +42:28:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212270_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212270_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 212227_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 212227_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 76035_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 76035_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 154939_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 154939_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 169509_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 169509_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
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Considering the candidate 155026_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
The candidate 155026_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287 did not pass the final checks
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Considering the candidate 167784_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
Preparing report for the candidate 167784_fd_Cyg-07-Q1b1x1_2026-05-19_01-56-56_20.00sec_-0.00C_LIGHTs_0287
make_report_in_HTML.sh Phase 2 (HTML assembly): 25s
make_report_in_HTML.sh TOTAL: 921s
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 ####
22:22:47.01 +32:45:45.7
22:23:06.21 +32:48:02.8
22:15:55.09 +33:10:18.4
22:18:38.88 +33:13:29.2
22:19:16.62 +33:14:56.7
22:18:38.97 +33:24:05.6
22:20:06.30 +33:26:31.1
22:18:40.15 +33:30:22.2
22:23:22.75 +33:27:23.4
22:14:30.42 +34:05:12.7
22:21:24.84 +40:44:14.8
22:24:47.82 +41:23:34.6
22:27:32.21 +40:12:34.8
22:20:34.56 +41:55:58.2
22:24:41.58 +41:00:04.8
22:24:04.58 +41:44:25.4
22:27:40.80 +38:24:06.8
22:28:14.10 +38:59:33.1
22:26:35.14 +36:30:44.8
22:27:58.20 +41:56:15.7
22:26:09.53 +39:20:23.0
22:28:59.62 +41:10:52.3
22:26:48.56 +40:52:45.3
22:25:31.35 +36:37:30.5
22:27:04.56 +36:34:03.6
22:26:22.08 +38:29:11.0
21:44:38.58 +38:02:24.8
21:23:29.50 +39:22:20.0
21:55:57.21 +40:10:26.6
21:10:17.90 +39:56:34.8
21:14:56.94 +37:19:03.4
22:01:22.40 +40:55:09.3
21:32:27.21 +38:28:54.9
21:36:54.23 +40:36:46.5
21:17:09.32 +42:14:59.2
21:42:55.18 +37:35:20.8
21:23:18.20 +42:11:40.3
21:20:22.07 +36:42:26.0
21:17:45.95 +35:45:18.2
21:34:37.49 +34:15:56.5
21:10:10.05 +42:07:59.7
21:48:47.05 +40:08:13.9
21:15:25.75 +36:10:50.0
22:14:40.29 +33:58:19.1
21:40:56.21 +41:13:24.8
21:12:34.00 +38:29:35.1
21:32:55.76 +38:02:35.9
22:05:39.71 +34:53:40.0
21:18:51.01 +34:56:41.1
21:27:23.91 +33:39:59.0
21:23:28.52 +42:28:11.4
21:41:19.29 +37:02:32.5
21:34:48.59 +33:48:32.7
21:17:20.43 +36:43:55.1
21:32:51.75 +35:15:27.0
21:20:25.16 +37:31:58.3
21:11:48.56 +37:16:05.0
21:28:11.80 +34:45:27.9
21:21:12.47 +36:20:38.0
21:22:57.41 +34:56:38.4
22:13:23.24 +33:35:20.4
21:35:00.60 +35:11:24.6
21:19:48.16 +37:09:11.9
22:00:18.66 +38:06:30.6
22:01:18.64 +41:30:28.5
22:12:38.32 +38:19:17.8
22:22:38.66 +33:28:06.7
22:19:05.13 +32:54:15.2
22:22:02.85 +32:44:45.0
22:22:13.30 +32:50:51.7
22:01:07.87 +39:15:18.6
22:18:24.32 +32:54:23.2
22:21:28.71 +32:41:44.2
22:23:54.63 +33:02:50.9
22:24:12.27 +32:53:19.9
22:19:19.12 +32:44:18.3
22:22:13.07 +32:41:36.1
22:21:18.80 +32:47:18.4
22:23:43.93 +33:23:34.1
22:24:02.20 +32:39:09.6
22:20:07.11 +32:50:48.7
22:24:47.50 +33:40:33.0
22:20:30.33 +32:41:34.8
21:31:14.81 +38:46:29.9
22:18:11.58 +32:43:33.2
22:23:12.48 +33:23:24.9
22:24:20.54 +32:49:58.8
22:20:10.09 +32:56:33.4
22:23:08.16 +32:50:44.2
22:22:11.78 +32:41:01.7
22:29:53.30 +41:26:00.2
22:23:07.72 +33:37:19.1
22:20:46.87 +32:50:51.1
22:18:46.75 +32:43:54.8
21:15:17.39 +38:56:43.9
22:23:11.20 +32:49:39.7
22:25:10.70 +33:50:28.1
22:23:49.51 +33:28:26.0
22:24:41.55 +33:06:45.4
22:22:56.89 +33:12:02.1
22:23:38.23 +33:32:00.0
22:17:38.58 +32:56:02.4
22:21:33.47 +32:52:45.0
22:24:05.46 +33:35:00.5
22:20:23.55 +33:06:53.7
22:24:20.52 +34:10:17.0
22:24:23.17 +33:12:16.0
22:20:28.76 +32:59:00.9
22:20:22.40 +32:56:11.9
22:23:07.16 +33:08:02.2
22:23:55.36 +34:07:37.3
22:22:50.68 +33:02:29.3
22:19:46.52 +33:02:15.5
21:42:50.22 +37:29:33.0
22:20:23.52 +32:54:15.2
22:24:35.31 +33:46:20.4
22:19:48.19 +33:01:21.3
22:19:14.40 +32:50:53.6
22:18:08.29 +32:50:45.1
21:27:28.55 +35:23:04.1
22:16:43.90 +33:05:24.7
22:23:44.34 +32:54:13.3
22:20:57.87 +32:46:23.1
21:21:47.69 +35:29:50.1
21:10:27.84 +36:47:46.3
22:18:25.16 +32:55:08.1
21:24:58.58 +36:59:14.2
22:20:34.59 +33:02:40.5
22:18:20.23 +32:53:58.5
22:22:33.42 +33:34:54.5
22:24:14.74 +33:37:32.5
22:20:37.31 +33:23:33.2
22:19:23.14 +32:59:21.0
22:24:27.88 +33:37:47.6
22:20:39.20 +32:54:15.2
22:20:39.00 +32:50:13.8
22:23:07.90 +33:23:02.6
21:50:26.30 +41:51:43.1
21:17:37.39 +36:35:15.8
22:23:02.72 +32:42:37.5
22:23:31.33 +32:43:59.5
21:29:32.56 +33:47:11.0
22:18:36.65 +32:58:58.0
22:20:45.94 +32:42:31.8
22:19:44.77 +33:18:41.9
22:20:50.94 +32:53:15.3
22:21:35.05 +32:41:15.4
21:22:36.14 +35:35:48.6
22:24:31.23 +34:22:25.5
22:21:46.71 +33:32:37.6
22:22:57.67 +33:36:03.3
22:11:47.62 +38:26:20.1
22:02:42.94 +33:22:25.8
22:22:28.49 +33:46:01.3
22:23:45.42 +33:03:10.9
22:23:27.37 +33:57:49.6
22:23:36.58 +33:39:32.2
22:24:19.63 +33:45:17.7
22:21:09.22 +33:14:22.0
22:22:51.88 +33:51:23.0
22:18:05.10 +32:44:50.7
21:42:45.65 +36:52:50.7
22:23:15.04 +34:07:35.0
22:19:32.53 +33:07:17.7
22:23:10.00 +34:09:20.1
22:21:07.21 +33:09:50.1
22:24:03.21 +33:02:09.1
21:26:25.10 +35:51:26.3
22:21:41.85 +33:15:31.7
21:26:53.13 +37:31:51.0
22:23:43.81 +33:04:00.7
22:22:08.94 +33:00:18.6
22:24:06.40 +33:47:07.0
22:23:20.66 +32:59:09.3
22:22:55.78 +33:33:57.5
21:23:35.23 +38:21:42.0
22:19:34.44 +33:14:38.1
22:20:56.39 +32:59:39.1
22:21:03.77 +33:12:54.3
22:22:19.37 +32:54:25.7
22:25:19.00 +34:03:17.2
22:23:25.02 +33:24:37.2
22:21:45.89 +33:23:34.6
22:19:23.99 +32:46:40.9
22:22:58.32 +32:58:41.8
22:24:08.92 +33:57:54.4
22:18:37.77 +32:48:16.6
21:13:10.67 +42:30:08.0
22:23:19.94 +33:27:41.0
22:20:40.74 +33:08:47.3
22:23:01.53 +32:54:18.4
21:15:42.98 +33:53:36.6
22:21:49.75 +33:05:15.9
22:20:21.50 +32:42:46.3
22:22:07.66 +32:48:47.3
22:19:10.61 +33:01:16.8
22:14:49.17 +32:48:44.8
21:31:02.09 +37:39:41.7
22:20:42.31 +33:18:15.6
22:23:55.51 +33:00:55.5
22:24:04.60 +34:24:03.0
22:19:26.54 +33:03:40.7
22:21:16.32 +33:39:10.4
22:20:55.87 +41:36:26.6
22:22:17.26 +32:41:43.5
22:24:46.42 +33:23:51.6
22:21:01.94 +33:19:23.0
21:17:44.52 +33:45:12.7
22:23:48.00 +33:17:20.9
22:23:48.10 +34:10:12.1
22:20:05.95 +32:43:47.6
21:34:48.86 +41:16:17.5
22:23:28.06 +32:56:28.4
21:40:40.87 +36:19:20.7
22:23:00.98 +33:29:38.4
21:41:29.00 +37:46:46.0
22:21:13.43 +32:41:43.0
21:24:39.30 +36:58:43.5
22:22:40.25 +34:04:04.1
22:20:39.92 +33:27:29.1
22:23:53.79 +32:58:14.7
21:32:54.29 +35:30:10.2
21:14:38.33 +37:33:54.1
22:23:42.36 +33:58:37.1
22:21:08.21 +33:31:44.5
22:07:05.37 +37:55:15.6
22:22:44.70 +33:19:20.4
22:21:27.93 +33:16:36.4
21:33:38.33 +37:37:18.2
21:31:28.39 +35:34:31.0
22:21:20.67 +32:54:29.7
22:21:52.14 +33:11:04.7
22:22:16.23 +33:18:12.1
22:22:03.92 +33:34:38.6
21:33:55.65 +39:39:30.3
22:25:05.76 +34:12:57.2
22:21:27.95 +33:30:51.2
22:22:33.50 +33:44:26.3
22:22:09.47 +32:46:04.4
22:22:40.12 +33:47:33.4
22:23:52.63 +33:08:36.3
22:21:41.06 +32:47:20.1
22:21:35.28 +33:45:23.8
22:24:13.04 +33:46:11.5
22:18:32.61 +32:45:57.5
22:24:02.73 +34:10:38.8
22:23:56.54 +33:46:36.7
22:20:22.16 +33:02:14.8
22:21:22.26 +32:51:29.8
21:16:00.24 +33:40:28.9
22:23:22.81 +32:55:55.3
22:24:16.55 +32:44:05.8
21:20:52.06 +38:17:40.1
21:25:56.61 +38:11:59.4
21:39:42.01 +39:56:25.6
21:14:44.97 +38:12:04.6
22:20:40.46 +33:17:26.4
22:21:08.78 +32:46:19.5
21:58:07.65 +38:56:43.1
22:21:26.71 +33:33:54.4
22:20:56.51 +33:12:56.9
22:23:24.36 +33:31:45.1
22:22:39.66 +33:39:09.3
21:35:16.60 +37:59:52.8
22:22:56.58 +33:21:10.8
22:24:48.21 +34:20:20.0
22:24:35.00 +33:07:57.2
22:21:43.44 +33:19:20.4
22:22:59.31 +33:34:17.8
22:01:53.20 +40:17:20.1
22:24:26.90 +33:02:13.5
22:23:34.30 +33:56:59.1
22:18:13.04 +32:48:49.6
22:23:41.27 +33:35:11.1
22:19:37.58 +42:13:56.2
22:22:30.21 +33:34:23.6
22:23:03.75 +33:14:11.5
22:24:57.77 +33:32:13.7
22:23:10.70 +33:50:35.1
22:24:39.03 +33:58:16.5
21:25:05.62 +37:46:27.9
22:22:12.35 +33:29:02.2
21:42:06.09 +36:50:54.1
22:21:30.33 +33:21:21.8
21:18:35.27 +40:16:40.9
22:23:37.08 +34:04:43.8
22:19:38.04 +33:02:55.3
22:21:05.10 +33:08:35.2
21:10:36.29 +40:19:48.4
22:17:57.51 +33:00:25.5
21:57:40.58 +37:18:46.3
22:21:11.00 +32:48:09.8
22:23:23.41 +33:32:22.9
22:18:18.44 +33:03:09.3
22:25:06.51 +33:54:39.9
21:42:46.24 +37:59:51.7
21:27:41.86 +38:45:47.5
22:23:40.39 +33:06:46.4
22:21:28.32 +33:30:23.0
22:24:04.84 +32:52:51.7
21:20:38.11 +36:33:48.2
22:22:28.49 +33:51:41.7
22:00:54.44 +41:16:16.1
22:23:44.96 +32:47:18.9
22:24:08.27 +33:27:45.7
22:25:04.56 +33:47:39.0
22:19:40.49 +33:14:50.8
22:22:31.67 +32:40:34.0
21:29:07.96 +42:01:04.7
22:18:42.70 +33:05:54.4
22:19:54.91 +32:47:47.2
22:20:47.78 +33:26:03.8
22:02:42.37 +41:44:11.1
22:22:23.71 +32:51:01.8
21:29:04.91 +40:27:04.7
22:19:44.20 +32:47:01.0
21:12:50.82 +36:08:09.5
22:25:35.96 +34:15:30.1
22:23:36.74 +33:59:16.9
22:21:41.54 +33:58:45.2
22:23:22.96 +33:18:06.0
22:23:49.40 +33:29:56.6
21:34:28.18 +39:24:27.9
22:24:01.94 +33:34:40.3
22:00:15.54 +42:40:25.6
22:20:18.57 +32:56:13.8
22:24:19.50 +33:47:17.9
21:33:38.97 +39:05:53.5
21:49:54.43 +34:54:45.8
22:19:14.02 +32:43:30.4
21:59:27.31 +38:47:13.7
22:01:13.39 +38:33:03.0
22:22:24.25 +33:43:44.1
22:19:18.86 +33:03:23.4
22:02:42.05 +37:08:58.3
22:07:49.39 +33:25:38.5
22:22:25.23 +32:47:16.9
22:04:54.80 +37:38:40.9
21:39:02.81 +40:22:36.4
21:52:08.98 +36:25:24.0
22:22:37.60 +33:42:30.3
22:03:59.82 +39:46:39.6
21:26:13.31 +36:37:42.3
22:23:00.58 +33:18:08.4
22:21:30.45 +33:24:03.5
22:18:38.59 +32:52:57.5
22:21:48.57 +33:16:34.8
22:22:28.70 +33:12:04.8
22:24:30.17 +33:12:13.8
22:06:46.39 +39:39:08.4
22:23:33.08 +32:55:50.5
22:22:24.55 +33:38:18.5
21:54:04.33 +37:39:40.0
22:21:33.24 +33:09:58.7
22:21:07.02 +32:55:56.2
22:20:44.06 +33:02:16.2
22:24:02.12 +33:51:15.8
22:19:12.03 +33:10:14.0
22:02:40.27 +38:06:45.8
21:37:56.45 +40:23:15.4
21:36:22.22 +40:35:08.1
21:27:59.75 +37:32:19.5
22:25:26.04 +34:33:53.2
21:42:23.04 +40:36:53.8
21:40:43.71 +37:23:00.9
21:35:18.47 +37:59:45.7
21:44:49.77 +36:56:55.2
22:14:26.75 +39:28:50.0
22:21:28.15 +33:14:45.2
22:21:50.53 +33:31:59.9
22:18:43.00 +33:06:49.5
22:23:10.54 +33:38:55.6
22:20:27.50 +33:24:46.9
22:20:27.28 +32:54:53.0
21:47:33.56 +37:22:57.0
22:22:11.83 +33:26:57.1
22:04:23.59 +39:34:07.2
22:21:49.31 +33:27:50.1
21:23:38.46 +35:00:20.4
21:52:06.19 +38:25:44.3
21:27:12.66 +39:53:03.7
21:49:54.34 +37:45:56.2
21:31:01.72 +37:20:11.1
22:24:46.92 +33:34:08.7
22:23:13.49 +34:11:34.8
22:23:01.57 +32:47:41.3
22:23:52.56 +33:21:51.6
21:29:41.41 +38:48:31.7
21:43:31.94 +38:44:14.3
22:24:50.18 +34:08:24.7
21:22:48.69 +36:59:06.2
22:19:31.08 +33:01:21.4
22:23:11.39 +33:56:44.8
22:23:44.35 +33:36:35.5
22:23:12.06 +34:06:18.2
21:52:14.84 +36:58:30.1
22:24:04.78 +33:37:06.6
21:59:59.99 +38:42:22.6
21:14:10.55 +37:06:09.8
21:10:16.65 +40:21:13.7
22:25:23.93 +34:23:42.5
22:05:01.78 +41:27:42.7
21:16:44.70 +42:11:22.0
21:27:03.51 +35:21:31.8
21:30:44.38 +35:40:19.5
21:22:09.19 +38:06:47.4
21:12:15.77 +41:54:51.6
22:02:41.35 +37:09:20.1
21:42:10.77 +39:16:10.7
21:44:26.63 +39:22:57.4
21:48:58.48 +37:54:22.4
21:42:45.53 +38:41:54.9
21:52:37.05 +39:29:23.8
21:59:24.47 +39:22:40.2
########### 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 ####
21:44:38.58 +38:02:24.8
21:23:29.50 +39:22:20.0
21:55:57.21 +40:10:26.6
21:10:17.90 +39:56:34.8
21:14:56.94 +37:19:03.4
22:01:22.40 +40:55:09.3
21:32:27.21 +38:28:54.9
21:36:54.23 +40:36:46.5
21:17:09.32 +42:14:59.2
21:42:55.18 +37:35:20.8
21:23:18.20 +42:11:40.3
21:20:22.07 +36:42:26.0
21:17:45.95 +35:45:18.2
21:34:37.49 +34:15:56.5
21:10:10.05 +42:07:59.7
21:48:47.05 +40:08:13.9
21:15:25.75 +36:10:50.0
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21:40:56.21 +41:13:24.8
21:12:34.00 +38:29:35.1
21:32:55.76 +38:02:35.9
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21:27:23.91 +33:39:59.0
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21:34:48.59 +33:48:32.7
21:17:20.43 +36:43:55.1
21:32:51.75 +35:15:27.0
21:20:25.16 +37:31:58.3
21:11:48.56 +37:16:05.0
21:28:11.80 +34:45:27.9
21:21:12.47 +36:20:38.0
21:22:57.41 +34:56:38.4
22:13:23.24 +33:35:20.4
21:35:00.60 +35:11:24.6
21:19:48.16 +37:09:11.9
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22:22:13.30 +32:50:51.7
22:01:07.87 +39:15:18.6
22:18:24.32 +32:54:23.2
22:21:28.71 +32:41:44.2
22:23:54.63 +33:02:50.9
22:24:12.27 +32:53:19.9
22:19:19.12 +32:44:18.3
22:22:13.07 +32:41:36.1
22:21:18.80 +32:47:18.4
22:23:43.93 +33:23:34.1
22:24:02.20 +32:39:09.6
22:20:07.11 +32:50:48.7
22:24:47.50 +33:40:33.0
22:20:30.33 +32:41:34.8
21:31:14.81 +38:46:29.9
22:18:11.58 +32:43:33.2
22:23:12.48 +33:23:24.9
22:24:20.54 +32:49:58.8
22:20:10.09 +32:56:33.4
22:23:08.16 +32:50:44.2
22:22:11.78 +32:41:01.7
22:29:53.30 +41:26:00.2
22:23:07.72 +33:37:19.1
22:20:46.87 +32:50:51.1
22:18:46.75 +32:43:54.8
21:15:17.39 +38:56:43.9
22:23:11.20 +32:49:39.7
22:25:10.70 +33:50:28.1
22:23:49.51 +33:28:26.0
22:24:41.55 +33:06:45.4
22:22:56.89 +33:12:02.1
22:23:38.23 +33:32:00.0
22:17:38.58 +32:56:02.4
22:21:33.47 +32:52:45.0
22:24:05.46 +33:35:00.5
22:20:23.55 +33:06:53.7
22:24:20.52 +34:10:17.0
22:24:23.17 +33:12:16.0
22:20:28.76 +32:59:00.9
22:20:22.40 +32:56:11.9
22:23:07.16 +33:08:02.2
22:23:55.36 +34:07:37.3
22:22:50.68 +33:02:29.3
22:19:46.52 +33:02:15.5
21:42:50.22 +37:29:33.0
22:20:23.52 +32:54:15.2
22:24:35.31 +33:46:20.4
22:19:48.19 +33:01:21.3
22:19:14.40 +32:50:53.6
22:18:08.29 +32:50:45.1
21:27:28.55 +35:23:04.1
22:16:43.90 +33:05:24.7
22:23:44.34 +32:54:13.3
22:20:57.87 +32:46:23.1
21:21:47.69 +35:29:50.1
21:10:27.84 +36:47:46.3
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21:24:58.58 +36:59:14.2
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21:17:37.39 +36:35:15.8
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21:29:32.56 +33:47:11.0
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21:26:25.10 +35:51:26.3
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21:26:53.13 +37:31:51.0
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22:22:08.94 +33:00:18.6
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21:23:35.23 +38:21:42.0
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21:31:02.09 +37:39:41.7
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22:20:55.87 +41:36:26.6
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22:21:01.94 +33:19:23.0
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21:34:48.86 +41:16:17.5
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21:40:40.87 +36:19:20.7
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21:41:29.00 +37:46:46.0
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21:24:39.30 +36:58:43.5
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21:32:54.29 +35:30:10.2
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21:33:55.65 +39:39:30.3
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22:18:18.44 +33:03:09.3
22:25:06.51 +33:54:39.9
21:42:46.24 +37:59:51.7
21:27:41.86 +38:45:47.5
22:23:40.39 +33:06:46.4
22:21:28.32 +33:30:23.0
22:24:04.84 +32:52:51.7
21:20:38.11 +36:33:48.2
22:22:28.49 +33:51:41.7
22:00:54.44 +41:16:16.1
22:23:44.96 +32:47:18.9
22:24:08.27 +33:27:45.7
22:25:04.56 +33:47:39.0
22:19:40.49 +33:14:50.8
22:22:31.67 +32:40:34.0
21:29:07.96 +42:01:04.7
22:18:42.70 +33:05:54.4
22:19:54.91 +32:47:47.2
22:20:47.78 +33:26:03.8
22:02:42.37 +41:44:11.1
22:22:23.71 +32:51:01.8
21:29:04.91 +40:27:04.7
22:19:44.20 +32:47:01.0
21:12:50.82 +36:08:09.5
22:25:35.96 +34:15:30.1
22:23:36.74 +33:59:16.9
22:21:41.54 +33:58:45.2
22:23:22.96 +33:18:06.0
22:23:49.40 +33:29:56.6
21:34:28.18 +39:24:27.9
22:24:01.94 +33:34:40.3
22:00:15.54 +42:40:25.6
22:20:18.57 +32:56:13.8
22:24:19.50 +33:47:17.9
21:33:38.97 +39:05:53.5
21:49:54.43 +34:54:45.8
22:19:14.02 +32:43:30.4
21:59:27.31 +38:47:13.7
22:01:13.39 +38:33:03.0
22:22:24.25 +33:43:44.1
22:19:18.86 +33:03:23.4
22:02:42.05 +37:08:58.3
22:07:49.39 +33:25:38.5
22:22:25.23 +32:47:16.9
22:04:54.80 +37:38:40.9
21:39:02.81 +40:22:36.4
21:52:08.98 +36:25:24.0
22:22:37.60 +33:42:30.3
22:03:59.82 +39:46:39.6
21:26:13.31 +36:37:42.3
22:23:00.58 +33:18:08.4
22:21:30.45 +33:24:03.5
22:18:38.59 +32:52:57.5
22:21:48.57 +33:16:34.8
22:22:28.70 +33:12:04.8
22:24:30.17 +33:12:13.8
22:06:46.39 +39:39:08.4
22:23:33.08 +32:55:50.5
22:22:24.55 +33:38:18.5
21:54:04.33 +37:39:40.0
22:21:33.24 +33:09:58.7
22:21:07.02 +32:55:56.2
22:20:44.06 +33:02:16.2
22:24:02.12 +33:51:15.8
22:19:12.03 +33:10:14.0
22:02:40.27 +38:06:45.8
21:37:56.45 +40:23:15.4
21:36:22.22 +40:35:08.1
21:27:59.75 +37:32:19.5
22:25:26.04 +34:33:53.2
21:42:23.04 +40:36:53.8
21:40:43.71 +37:23:00.9
21:35:18.47 +37:59:45.7
21:44:49.77 +36:56:55.2
22:14:26.75 +39:28:50.0
22:21:28.15 +33:14:45.2
22:21:50.53 +33:31:59.9
22:18:43.00 +33:06:49.5
22:23:10.54 +33:38:55.6
22:20:27.50 +33:24:46.9
22:20:27.28 +32:54:53.0
21:47:33.56 +37:22:57.0
22:22:11.83 +33:26:57.1
22:04:23.59 +39:34:07.2
22:21:49.31 +33:27:50.1
21:23:38.46 +35:00:20.4
21:52:06.19 +38:25:44.3
21:27:12.66 +39:53:03.7
21:49:54.34 +37:45:56.2
21:31:01.72 +37:20:11.1
22:24:46.92 +33:34:08.7
22:23:13.49 +34:11:34.8
22:23:01.57 +32:47:41.3
22:23:52.56 +33:21:51.6
21:29:41.41 +38:48:31.7
21:43:31.94 +38:44:14.3
22:24:50.18 +34:08:24.7
21:22:48.69 +36:59:06.2
22:19:31.08 +33:01:21.4
22:23:11.39 +33:56:44.8
22:23:44.35 +33:36:35.5
22:23:12.06 +34:06:18.2
21:52:14.84 +36:58:30.1
22:24:04.78 +33:37:06.6
21:59:59.99 +38:42:22.6
21:14:10.55 +37:06:09.8
21:10:16.65 +40:21:13.7
22:25:23.93 +34:23:42.5
22:05:01.78 +41:27:42.7
21:16:44.70 +42:11:22.0
21:27:03.51 +35:21:31.8
21:30:44.38 +35:40:19.5
21:22:09.19 +38:06:47.4
21:12:15.77 +41:54:51.6
22:02:41.35 +37:09:20.1
21:42:10.77 +39:16:10.7
21:44:26.63 +39:22:57.4
21:48:58.48 +37:54:22.4
21:42:45.53 +38:41:54.9
22:23:06.21 +32:48:02.8
22:24:47.82 +41:23:34.6
22:14:30.42 +34:05:12.7
22:20:06.30 +33:26:31.1
21:52:37.05 +39:29:23.8
22:18:38.88 +33:13:29.2
22:22:47.01 +32:45:45.7
22:19:16.62 +33:14:56.7
22:26:22.08 +38:29:11.0
22:27:04.56 +36:34:03.6
22:25:31.35 +36:37:30.5
22:26:48.56 +40:52:45.3
22:28:59.62 +41:10:52.3
22:26:09.53 +39:20:23.0
22:23:22.75 +33:27:23.4
22:27:58.20 +41:56:15.7
22:26:35.14 +36:30:44.8
22:28:14.10 +38:59:33.1
22:27:40.80 +38:24:06.8
22:24:04.58 +41:44:25.4
22:15:55.09 +33:10:18.4
22:24:41.58 +41:00:04.8
22:20:34.56 +41:55:58.2
22:27:32.21 +40:12:34.8
22:21:24.84 +40:44:14.8
21:59:24.47 +39:22:40.2
22:18:40.15 +33:30:22.2
22:18:38.97 +33:24:05.6
###################################################################################
21:44:38.58 +38:02:24.8 -- not an asteroid (will add it to exclusion list)
21:23:29.50 +39:22:20.0 -- not an asteroid (will add it to exclusion list)
21:55:57.21 +40:10:26.6 -- not an asteroid (will add it to exclusion list)
21:10:17.90 +39:56:34.8 -- not an asteroid (will add it to exclusion list)
21:14:56.94 +37:19:03.4 -- not an asteroid (will add it to exclusion list)
22:01:22.40 +40:55:09.3 -- not an asteroid (will add it to exclusion list)
21:32:27.21 +38:28:54.9 -- not an asteroid (will add it to exclusion list)
21:36:54.23 +40:36:46.5 -- not an asteroid (will add it to exclusion list)
21:17:09.32 +42:14:59.2 -- not an asteroid (will add it to exclusion list)
21:42:55.18 +37:35:20.8 -- not an asteroid (will add it to exclusion list)
21:23:18.20 +42:11:40.3 -- not an asteroid (will add it to exclusion list)
21:20:22.07 +36:42:26.0 -- not an asteroid (will add it to exclusion list)
21:17:45.95 +35:45:18.2 -- not an asteroid (will add it to exclusion list)
21:34:37.49 +34:15:56.5 -- not an asteroid (will add it to exclusion list)
21:10:10.05 +42:07:59.7 -- not an asteroid (will add it to exclusion list)
21:48:47.05 +40:08:13.9 -- not an asteroid (will add it to exclusion list)
21:15:25.75 +36:10:50.0 -- not an asteroid (will add it to exclusion list)
22:14:40.29 +33:58:19.1 -- not an asteroid (will add it to exclusion list)
21:40:56.21 +41:13:24.8 -- not an asteroid (will add it to exclusion list)
21:12:34.00 +38:29:35.1 -- not an asteroid (will add it to exclusion list)
21:32:55.76 +38:02:35.9 -- not an asteroid (will add it to exclusion list)
22:05:39.71 +34:53:40.0 -- not an asteroid (will add it to exclusion list)
21:18:51.01 +34:56:41.1 -- not an asteroid (will add it to exclusion list)
21:27:23.91 +33:39:59.0 -- not an asteroid (will add it to exclusion list)
21:23:28.52 +42:28:11.4 -- not an asteroid (will add it to exclusion list)
21:41:19.29 +37:02:32.5 -- not an asteroid (will add it to exclusion list)
21:34:48.59 +33:48:32.7 -- not an asteroid (will add it to exclusion list)
21:17:20.43 +36:43:55.1 -- not an asteroid (will add it to exclusion list)
21:32:51.75 +35:15:27.0 -- not an asteroid (will add it to exclusion list)
21:20:25.16 +37:31:58.3 -- not an asteroid (will add it to exclusion list)
21:11:48.56 +37:16:05.0 -- not an asteroid (will add it to exclusion list)
21:28:11.80 +34:45:27.9 -- not an asteroid (will add it to exclusion list)
21:21:12.47 +36:20:38.0 -- not an asteroid (will add it to exclusion list)
21:22:57.41 +34:56:38.4 -- not an asteroid (will add it to exclusion list)
22:13:23.24 +33:35:20.4 -- not an asteroid (will add it to exclusion list)
21:35:00.60 +35:11:24.6 -- not an asteroid (will add it to exclusion list)
21:19:48.16 +37:09:11.9 -- not an asteroid (will add it to exclusion list)
22:00:18.66 +38:06:30.6 -- not an asteroid (will add it to exclusion list)
22:01:18.64 +41:30:28.5 -- not an asteroid (will add it to exclusion list)
22:12:38.32 +38:19:17.8 -- not an asteroid (will add it to exclusion list)
22:22:38.66 +33:28:06.7 -- not an asteroid (will add it to exclusion list)
22:19:05.13 +32:54:15.2 -- not an asteroid (will add it to exclusion list)
22:22:02.85 +32:44:45.0 -- not an asteroid (will add it to exclusion list)
22:22:13.30 +32:50:51.7 -- not an asteroid (will add it to exclusion list)
22:01:07.87 +39:15:18.6 -- not an asteroid (will add it to exclusion list)
22:18:24.32 +32:54:23.2 -- not an asteroid (will add it to exclusion list)
22:21:28.71 +32:41:44.2 -- not an asteroid (will add it to exclusion list)
22:23:54.63 +33:02:50.9 -- not an asteroid (will add it to exclusion list)
22:24:12.27 +32:53:19.9 -- not an asteroid (will add it to exclusion list)
22:19:19.12 +32:44:18.3 -- not an asteroid (will add it to exclusion list)
22:22:13.07 +32:41:36.1 -- not an asteroid (will add it to exclusion list)
22:21:18.80 +32:47:18.4 -- not an asteroid (will add it to exclusion list)
22:23:43.93 +33:23:34.1 -- not an asteroid (will add it to exclusion list)
22:24:02.20 +32:39:09.6 -- not an asteroid (will add it to exclusion list)
22:20:07.11 +32:50:48.7 -- not an asteroid (will add it to exclusion list)
22:24:47.50 +33:40:33.0 -- not an asteroid (will add it to exclusion list)
22:20:30.33 +32:41:34.8 -- not an asteroid (will add it to exclusion list)
21:31:14.81 +38:46:29.9 -- not an asteroid (will add it to exclusion list)
22:18:11.58 +32:43:33.2 -- not an asteroid (will add it to exclusion list)
22:23:12.48 +33:23:24.9 -- not an asteroid (will add it to exclusion list)
22:24:20.54 +32:49:58.8 -- not an asteroid (will add it to exclusion list)
22:20:10.09 +32:56:33.4 -- not an asteroid (will add it to exclusion list)
22:23:08.16 +32:50:44.2 -- not an asteroid (will add it to exclusion list)
22:22:11.78 +32:41:01.7 -- not an asteroid (will add it to exclusion list)
22:29:53.30 +41:26:00.2 -- not an asteroid (will add it to exclusion list)
22:23:07.72 +33:37:19.1 -- not an asteroid (will add it to exclusion list)
22:20:46.87 +32:50:51.1 -- not an asteroid (will add it to exclusion list)
22:18:46.75 +32:43:54.8 -- not an asteroid (will add it to exclusion list)
21:15:17.39 +38:56:43.9 -- not an asteroid (will add it to exclusion list)
22:23:11.20 +32:49:39.7 -- not an asteroid (will add it to exclusion list)
22:25:10.70 +33:50:28.1 -- not an asteroid (will add it to exclusion list)
22:23:49.51 +33:28:26.0 -- not an asteroid (will add it to exclusion list)
22:24:41.55 +33:06:45.4 -- not an asteroid (will add it to exclusion list)
22:22:56.89 +33:12:02.1 -- not an asteroid (will add it to exclusion list)
22:23:38.23 +33:32:00.0 -- not an asteroid (will add it to exclusion list)
22:17:38.58 +32:56:02.4 -- not an asteroid (will add it to exclusion list)
22:21:33.47 +32:52:45.0 -- not an asteroid (will add it to exclusion list)
22:24:05.46 +33:35:00.5 -- not an asteroid (will add it to exclusion list)
22:20:23.55 +33:06:53.7 -- not an asteroid (will add it to exclusion list)
22:24:20.52 +34:10:17.0 -- not an asteroid (will add it to exclusion list)
22:24:23.17 +33:12:16.0 -- not an asteroid (will add it to exclusion list)
22:20:28.76 +32:59:00.9 -- not an asteroid (will add it to exclusion list)
22:20:22.40 +32:56:11.9 -- not an asteroid (will add it to exclusion list)
22:23:07.16 +33:08:02.2 -- not an asteroid (will add it to exclusion list)
22:23:55.36 +34:07:37.3 -- not an asteroid (will add it to exclusion list)
22:22:50.68 +33:02:29.3 -- not an asteroid (will add it to exclusion list)
22:19:46.52 +33:02:15.5 -- not an asteroid (will add it to exclusion list)
21:42:50.22 +37:29:33.0 -- not an asteroid (will add it to exclusion list)
22:20:23.52 +32:54:15.2 -- not an asteroid (will add it to exclusion list)
22:24:35.31 +33:46:20.4 -- not an asteroid (will add it to exclusion list)
22:19:48.19 +33:01:21.3 -- not an asteroid (will add it to exclusion list)
22:19:14.40 +32:50:53.6 -- not an asteroid (will add it to exclusion list)
22:18:08.29 +32:50:45.1 -- not an asteroid (will add it to exclusion list)
21:27:28.55 +35:23:04.1 -- not an asteroid (will add it to exclusion list)
22:16:43.90 +33:05:24.7 -- not an asteroid (will add it to exclusion list)
22:23:44.34 +32:54:13.3 -- not an asteroid (will add it to exclusion list)
22:20:57.87 +32:46:23.1 -- not an asteroid (will add it to exclusion list)
21:21:47.69 +35:29:50.1 -- not an asteroid (will add it to exclusion list)
21:10:27.84 +36:47:46.3 -- not an asteroid (will add it to exclusion list)
22:18:25.16 +32:55:08.1 -- not an asteroid (will add it to exclusion list)
21:24:58.58 +36:59:14.2 -- not an asteroid (will add it to exclusion list)
22:20:34.59 +33:02:40.5 -- not an asteroid (will add it to exclusion list)
22:18:20.23 +32:53:58.5 -- not an asteroid (will add it to exclusion list)
22:22:33.42 +33:34:54.5 -- not an asteroid (will add it to exclusion list)
22:24:14.74 +33:37:32.5 -- not an asteroid (will add it to exclusion list)
22:20:37.31 +33:23:33.2 -- not an asteroid (will add it to exclusion list)
22:19:23.14 +32:59:21.0 -- not an asteroid (will add it to exclusion list)
22:24:27.88 +33:37:47.6 -- not an asteroid (will add it to exclusion list)
22:20:39.20 +32:54:15.2 -- not an asteroid (will add it to exclusion list)
22:20:39.00 +32:50:13.8 -- not an asteroid (will add it to exclusion list)
22:23:07.90 +33:23:02.6 -- not an asteroid (will add it to exclusion list)
21:50:26.30 +41:51:43.1 -- not an asteroid (will add it to exclusion list)
21:17:37.39 +36:35:15.8 -- not an asteroid (will add it to exclusion list)
22:23:02.72 +32:42:37.5 -- not an asteroid (will add it to exclusion list)
22:23:31.33 +32:43:59.5 -- not an asteroid (will add it to exclusion list)
21:29:32.56 +33:47:11.0 -- not an asteroid (will add it to exclusion list)
22:18:36.65 +32:58:58.0 -- not an asteroid (will add it to exclusion list)
22:20:45.94 +32:42:31.8 -- not an asteroid (will add it to exclusion list)
22:19:44.77 +33:18:41.9 -- not an asteroid (will add it to exclusion list)
22:20:50.94 +32:53:15.3 -- not an asteroid (will add it to exclusion list)
22:21:35.05 +32:41:15.4 -- not an asteroid (will add it to exclusion list)
21:22:36.14 +35:35:48.6 -- not an asteroid (will add it to exclusion list)
22:24:31.23 +34:22:25.5 -- not an asteroid (will add it to exclusion list)
22:21:46.71 +33:32:37.6 -- not an asteroid (will add it to exclusion list)
22:22:57.67 +33:36:03.3 -- not an asteroid (will add it to exclusion list)
22:11:47.62 +38:26:20.1 -- not an asteroid (will add it to exclusion list)
22:02:42.94 +33:22:25.8 -- not an asteroid (will add it to exclusion list)
22:22:28.49 +33:46:01.3 -- not an asteroid (will add it to exclusion list)
22:23:45.42 +33:03:10.9 -- not an asteroid (will add it to exclusion list)
22:23:27.37 +33:57:49.6 -- not an asteroid (will add it to exclusion list)
22:23:36.58 +33:39:32.2 -- not an asteroid (will add it to exclusion list)
22:24:19.63 +33:45:17.7 -- not an asteroid (will add it to exclusion list)
22:21:09.22 +33:14:22.0 -- not an asteroid (will add it to exclusion list)
22:22:51.88 +33:51:23.0 -- not an asteroid (will add it to exclusion list)
22:18:05.10 +32:44:50.7 -- not an asteroid (will add it to exclusion list)
21:42:45.65 +36:52:50.7 -- not an asteroid (will add it to exclusion list)
22:23:15.04 +34:07:35.0 -- not an asteroid (will add it to exclusion list)
22:19:32.53 +33:07:17.7 -- not an asteroid (will add it to exclusion list)
22:23:10.00 +34:09:20.1 -- not an asteroid (will add it to exclusion list)
22:21:07.21 +33:09:50.1 -- not an asteroid (will add it to exclusion list)
22:24:03.21 +33:02:09.1 -- not an asteroid (will add it to exclusion list)
21:26:25.10 +35:51:26.3 -- not an asteroid (will add it to exclusion list)
22:21:41.85 +33:15:31.7 -- not an asteroid (will add it to exclusion list)
21:26:53.13 +37:31:51.0 -- not an asteroid (will add it to exclusion list)
22:23:43.81 +33:04:00.7 -- not an asteroid (will add it to exclusion list)
22:22:08.94 +33:00:18.6 -- not an asteroid (will add it to exclusion list)
22:24:06.40 +33:47:07.0 -- not an asteroid (will add it to exclusion list)
22:23:20.66 +32:59:09.3 -- not an asteroid (will add it to exclusion list)
22:22:55.78 +33:33:57.5 -- not an asteroid (will add it to exclusion list)
21:23:35.23 +38:21:42.0 -- not an asteroid (will add it to exclusion list)
22:19:34.44 +33:14:38.1 -- not an asteroid (will add it to exclusion list)
22:20:56.39 +32:59:39.1 -- not an asteroid (will add it to exclusion list)
22:21:03.77 +33:12:54.3 -- not an asteroid (will add it to exclusion list)
22:22:19.37 +32:54:25.7 -- not an asteroid (will add it to exclusion list)
22:25:19.00 +34:03:17.2 -- not an asteroid (will add it to exclusion list)
22:23:25.02 +33:24:37.2 -- not an asteroid (will add it to exclusion list)
22:21:45.89 +33:23:34.6 -- not an asteroid (will add it to exclusion list)
22:19:23.99 +32:46:40.9 -- not an asteroid (will add it to exclusion list)
22:22:58.32 +32:58:41.8 -- not an asteroid (will add it to exclusion list)
22:24:08.92 +33:57:54.4 -- not an asteroid (will add it to exclusion list)
22:18:37.77 +32:48:16.6 -- not an asteroid (will add it to exclusion list)
21:13:10.67 +42:30:08.0 -- not an asteroid (will add it to exclusion list)
22:23:19.94 +33:27:41.0 -- not an asteroid (will add it to exclusion list)
22:20:40.74 +33:08:47.3 -- not an asteroid (will add it to exclusion list)
22:23:01.53 +32:54:18.4 -- not an asteroid (will add it to exclusion list)
21:15:42.98 +33:53:36.6 -- not an asteroid (will add it to exclusion list)
22:21:49.75 +33:05:15.9 -- not an asteroid (will add it to exclusion list)
22:20:21.50 +32:42:46.3 -- not an asteroid (will add it to exclusion list)
22:22:07.66 +32:48:47.3 -- not an asteroid (will add it to exclusion list)
22:19:10.61 +33:01:16.8 -- not an asteroid (will add it to exclusion list)
22:14:49.17 +32:48:44.8 -- not an asteroid (will add it to exclusion list)
21:31:02.09 +37:39:41.7 -- not an asteroid (will add it to exclusion list)
22:20:42.31 +33:18:15.6 -- not an asteroid (will add it to exclusion list)
22:23:55.51 +33:00:55.5 -- not an asteroid (will add it to exclusion list)
22:24:04.60 +34:24:03.0 -- not an asteroid (will add it to exclusion list)
22:19:26.54 +33:03:40.7 -- not an asteroid (will add it to exclusion list)
22:21:16.32 +33:39:10.4 -- not an asteroid (will add it to exclusion list)
22:20:55.87 +41:36:26.6 -- not an asteroid (will add it to exclusion list)
22:22:17.26 +32:41:43.5 -- not an asteroid (will add it to exclusion list)
22:24:46.42 +33:23:51.6 -- not an asteroid (will add it to exclusion list)
22:21:01.94 +33:19:23.0 -- not an asteroid (will add it to exclusion list)
21:17:44.52 +33:45:12.7 -- not an asteroid (will add it to exclusion list)
22:23:48.00 +33:17:20.9 -- not an asteroid (will add it to exclusion list)
22:23:48.10 +34:10:12.1 -- not an asteroid (will add it to exclusion list)
22:20:05.95 +32:43:47.6 -- not an asteroid (will add it to exclusion list)
21:34:48.86 +41:16:17.5 -- not an asteroid (will add it to exclusion list)
22:23:28.06 +32:56:28.4 -- not an asteroid (will add it to exclusion list)
21:40:40.87 +36:19:20.7 -- not an asteroid (will add it to exclusion list)
22:23:00.98 +33:29:38.4 -- not an asteroid (will add it to exclusion list)
21:41:29.00 +37:46:46.0 -- not an asteroid (will add it to exclusion list)
22:21:13.43 +32:41:43.0 -- not an asteroid (will add it to exclusion list)
21:24:39.30 +36:58:43.5 -- not an asteroid (will add it to exclusion list)
22:22:40.25 +34:04:04.1 -- not an asteroid (will add it to exclusion list)
22:20:39.92 +33:27:29.1 -- not an asteroid (will add it to exclusion list)
22:23:53.79 +32:58:14.7 -- not an asteroid (will add it to exclusion list)
21:32:54.29 +35:30:10.2 -- not an asteroid (will add it to exclusion list)
21:14:38.33 +37:33:54.1 -- not an asteroid (will add it to exclusion list)
22:23:42.36 +33:58:37.1 -- not an asteroid (will add it to exclusion list)
22:21:08.21 +33:31:44.5 -- not an asteroid (will add it to exclusion list)
22:07:05.37 +37:55:15.6 -- not an asteroid (will add it to exclusion list)
22:22:44.70 +33:19:20.4 -- not an asteroid (will add it to exclusion list)
22:21:27.93 +33:16:36.4 -- not an asteroid (will add it to exclusion list)
21:33:38.33 +37:37:18.2 -- not an asteroid (will add it to exclusion list)
21:31:28.39 +35:34:31.0 -- not an asteroid (will add it to exclusion list)
22:21:20.67 +32:54:29.7 -- not an asteroid (will add it to exclusion list)
22:21:52.14 +33:11:04.7 -- not an asteroid (will add it to exclusion list)
22:22:16.23 +33:18:12.1 -- not an asteroid (will add it to exclusion list)
22:22:03.92 +33:34:38.6 -- not an asteroid (will add it to exclusion list)
21:33:55.65 +39:39:30.3 -- not an asteroid (will add it to exclusion list)
22:25:05.76 +34:12:57.2 -- not an asteroid (will add it to exclusion list)
22:21:27.95 +33:30:51.2 -- not an asteroid (will add it to exclusion list)
22:22:33.50 +33:44:26.3 -- not an asteroid (will add it to exclusion list)
22:22:09.47 +32:46:04.4 -- not an asteroid (will add it to exclusion list)
22:22:40.12 +33:47:33.4 -- not an asteroid (will add it to exclusion list)
22:23:52.63 +33:08:36.3 -- not an asteroid (will add it to exclusion list)
22:21:41.06 +32:47:20.1 -- not an asteroid (will add it to exclusion list)
22:21:35.28 +33:45:23.8 -- not an asteroid (will add it to exclusion list)
22:24:13.04 +33:46:11.5 -- not an asteroid (will add it to exclusion list)
22:18:32.61 +32:45:57.5 -- not an asteroid (will add it to exclusion list)
22:24:02.73 +34:10:38.8 -- not an asteroid (will add it to exclusion list)
22:23:56.54 +33:46:36.7 -- not an asteroid (will add it to exclusion list)
22:20:22.16 +33:02:14.8 -- not an asteroid (will add it to exclusion list)
22:21:22.26 +32:51:29.8 -- not an asteroid (will add it to exclusion list)
21:16:00.24 +33:40:28.9 -- not an asteroid (will add it to exclusion list)
22:23:22.81 +32:55:55.3 -- not an asteroid (will add it to exclusion list)
22:24:16.55 +32:44:05.8 -- not an asteroid (will add it to exclusion list)
21:20:52.06 +38:17:40.1 -- not an asteroid (will add it to exclusion list)
21:25:56.61 +38:11:59.4 -- not an asteroid (will add it to exclusion list)
21:39:42.01 +39:56:25.6 -- not an asteroid (will add it to exclusion list)
21:14:44.97 +38:12:04.6 -- not an asteroid (will add it to exclusion list)
22:20:40.46 +33:17:26.4 -- not an asteroid (will add it to exclusion list)
22:21:08.78 +32:46:19.5 -- not an asteroid (will add it to exclusion list)
21:58:07.65 +38:56:43.1 -- not an asteroid (will add it to exclusion list)
22:21:26.71 +33:33:54.4 -- not an asteroid (will add it to exclusion list)
22:20:56.51 +33:12:56.9 -- not an asteroid (will add it to exclusion list)
22:23:24.36 +33:31:45.1 -- not an asteroid (will add it to exclusion list)
22:22:39.66 +33:39:09.3 -- not an asteroid (will add it to exclusion list)
21:35:16.60 +37:59:52.8 -- not an asteroid (will add it to exclusion list)
22:22:56.58 +33:21:10.8 -- not an asteroid (will add it to exclusion list)
22:24:48.21 +34:20:20.0 -- not an asteroid (will add it to exclusion list)
22:24:35.00 +33:07:57.2 -- not an asteroid (will add it to exclusion list)
22:21:43.44 +33:19:20.4 -- not an asteroid (will add it to exclusion list)
22:22:59.31 +33:34:17.8 -- not an asteroid (will add it to exclusion list)
22:01:53.20 +40:17:20.1 -- not an asteroid (will add it to exclusion list)
22:24:26.90 +33:02:13.5 -- not an asteroid (will add it to exclusion list)
22:23:34.30 +33:56:59.1 -- not an asteroid (will add it to exclusion list)
22:18:13.04 +32:48:49.6 -- not an asteroid (will add it to exclusion list)
22:23:41.27 +33:35:11.1 -- not an asteroid (will add it to exclusion list)
22:19:37.58 +42:13:56.2 -- not an asteroid (will add it to exclusion list)
22:22:30.21 +33:34:23.6 -- not an asteroid (will add it to exclusion list)
22:23:03.75 +33:14:11.5 -- not an asteroid (will add it to exclusion list)
22:24:57.77 +33:32:13.7 -- not an asteroid (will add it to exclusion list)
22:23:10.70 +33:50:35.1 -- not an asteroid (will add it to exclusion list)
22:24:39.03 +33:58:16.5 -- not an asteroid (will add it to exclusion list)
21:25:05.62 +37:46:27.9 -- not an asteroid (will add it to exclusion list)
22:22:12.35 +33:29:02.2 -- not an asteroid (will add it to exclusion list)
21:42:06.09 +36:50:54.1 -- not an asteroid (will add it to exclusion list)
22:21:30.33 +33:21:21.8 -- not an asteroid (will add it to exclusion list)
21:18:35.27 +40:16:40.9 -- not an asteroid (will add it to exclusion list)
22:23:37.08 +34:04:43.8 -- not an asteroid (will add it to exclusion list)
22:19:38.04 +33:02:55.3 -- not an asteroid (will add it to exclusion list)
22:21:05.10 +33:08:35.2 -- not an asteroid (will add it to exclusion list)
21:10:36.29 +40:19:48.4 -- not an asteroid (will add it to exclusion list)
22:17:57.51 +33:00:25.5 -- not an asteroid (will add it to exclusion list)
21:57:40.58 +37:18:46.3 -- not an asteroid (will add it to exclusion list)
22:21:11.00 +32:48:09.8 -- not an asteroid (will add it to exclusion list)
22:23:23.41 +33:32:22.9 -- not an asteroid (will add it to exclusion list)
22:18:18.44 +33:03:09.3 -- not an asteroid (will add it to exclusion list)
22:25:06.51 +33:54:39.9 -- not an asteroid (will add it to exclusion list)
21:42:46.24 +37:59:51.7 -- not an asteroid (will add it to exclusion list)
21:27:41.86 +38:45:47.5 -- not an asteroid (will add it to exclusion list)
22:23:40.39 +33:06:46.4 -- not an asteroid (will add it to exclusion list)
22:21:28.32 +33:30:23.0 -- not an asteroid (will add it to exclusion list)
22:24:04.84 +32:52:51.7 -- not an asteroid (will add it to exclusion list)
21:20:38.11 +36:33:48.2 -- not an asteroid (will add it to exclusion list)
22:22:28.49 +33:51:41.7 -- not an asteroid (will add it to exclusion list)
22:00:54.44 +41:16:16.1 -- not an asteroid (will add it to exclusion list)
22:23:44.96 +32:47:18.9 -- not an asteroid (will add it to exclusion list)
22:24:08.27 +33:27:45.7 -- not an asteroid (will add it to exclusion list)
22:25:04.56 +33:47:39.0 -- not an asteroid (will add it to exclusion list)
22:19:40.49 +33:14:50.8 -- not an asteroid (will add it to exclusion list)
22:22:31.67 +32:40:34.0 -- not an asteroid (will add it to exclusion list)
21:29:07.96 +42:01:04.7 -- not an asteroid (will add it to exclusion list)
22:18:42.70 +33:05:54.4 -- not an asteroid (will add it to exclusion list)
22:19:54.91 +32:47:47.2 -- not an asteroid (will add it to exclusion list)
22:20:47.78 +33:26:03.8 -- not an asteroid (will add it to exclusion list)
22:02:42.37 +41:44:11.1 -- not an asteroid (will add it to exclusion list)
22:22:23.71 +32:51:01.8 -- not an asteroid (will add it to exclusion list)
21:29:04.91 +40:27:04.7 -- not an asteroid (will add it to exclusion list)
22:19:44.20 +32:47:01.0 -- not an asteroid (will add it to exclusion list)
21:12:50.82 +36:08:09.5 -- not an asteroid (will add it to exclusion list)
22:25:35.96 +34:15:30.1 -- not an asteroid (will add it to exclusion list)
22:23:36.74 +33:59:16.9 -- not an asteroid (will add it to exclusion list)
22:21:41.54 +33:58:45.2 -- not an asteroid (will add it to exclusion list)
22:23:22.96 +33:18:06.0 -- not an asteroid (will add it to exclusion list)
22:23:49.40 +33:29:56.6 -- not an asteroid (will add it to exclusion list)
21:34:28.18 +39:24:27.9 -- not an asteroid (will add it to exclusion list)
22:24:01.94 +33:34:40.3 -- not an asteroid (will add it to exclusion list)
22:00:15.54 +42:40:25.6 -- not an asteroid (will add it to exclusion list)
22:20:18.57 +32:56:13.8 -- not an asteroid (will add it to exclusion list)
22:24:19.50 +33:47:17.9 -- not an asteroid (will add it to exclusion list)
21:33:38.97 +39:05:53.5 -- not an asteroid (will add it to exclusion list)
21:49:54.43 +34:54:45.8 -- not an asteroid (will add it to exclusion list)
22:19:14.02 +32:43:30.4 -- not an asteroid (will add it to exclusion list)
21:59:27.31 +38:47:13.7 -- not an asteroid (will add it to exclusion list)
22:01:13.39 +38:33:03.0 -- not an asteroid (will add it to exclusion list)
22:22:24.25 +33:43:44.1 -- not an asteroid (will add it to exclusion list)
22:19:18.86 +33:03:23.4 -- not an asteroid (will add it to exclusion list)
22:02:42.05 +37:08:58.3 -- not an asteroid (will add it to exclusion list)
22:07:49.39 +33:25:38.5 -- not an asteroid (will add it to exclusion list)
22:22:25.23 +32:47:16.9 -- not an asteroid (will add it to exclusion list)
22:04:54.80 +37:38:40.9 -- not an asteroid (will add it to exclusion list)
21:39:02.81 +40:22:36.4 -- not an asteroid (will add it to exclusion list)
21:52:08.98 +36:25:24.0 -- not an asteroid (will add it to exclusion list)
22:22:37.60 +33:42:30.3 -- not an asteroid (will add it to exclusion list)
22:03:59.82 +39:46:39.6 -- not an asteroid (will add it to exclusion list)
21:26:13.31 +36:37:42.3 -- not an asteroid (will add it to exclusion list)
22:23:00.58 +33:18:08.4 -- not an asteroid (will add it to exclusion list)
22:21:30.45 +33:24:03.5 -- not an asteroid (will add it to exclusion list)
22:18:38.59 +32:52:57.5 -- not an asteroid (will add it to exclusion list)
22:21:48.57 +33:16:34.8 -- not an asteroid (will add it to exclusion list)
22:22:28.70 +33:12:04.8 -- not an asteroid (will add it to exclusion list)
22:24:30.17 +33:12:13.8 -- not an asteroid (will add it to exclusion list)
22:06:46.39 +39:39:08.4 -- not an asteroid (will add it to exclusion list)
22:23:33.08 +32:55:50.5 -- not an asteroid (will add it to exclusion list)
22:22:24.55 +33:38:18.5 -- not an asteroid (will add it to exclusion list)
21:54:04.33 +37:39:40.0 -- not an asteroid (will add it to exclusion list)
22:21:33.24 +33:09:58.7 -- not an asteroid (will add it to exclusion list)
22:21:07.02 +32:55:56.2 -- not an asteroid (will add it to exclusion list)
22:20:44.06 +33:02:16.2 -- not an asteroid (will add it to exclusion list)
22:24:02.12 +33:51:15.8 -- not an asteroid (will add it to exclusion list)
22:19:12.03 +33:10:14.0 -- not an asteroid (will add it to exclusion list)
22:02:40.27 +38:06:45.8 -- not an asteroid (will add it to exclusion list)
21:37:56.45 +40:23:15.4 -- not an asteroid (will add it to exclusion list)
21:36:22.22 +40:35:08.1 -- not an asteroid (will add it to exclusion list)
21:27:59.75 +37:32:19.5 -- not an asteroid (will add it to exclusion list)
22:25:26.04 +34:33:53.2 -- not an asteroid (will add it to exclusion list)
21:42:23.04 +40:36:53.8 -- not an asteroid (will add it to exclusion list)
21:40:43.71 +37:23:00.9 -- not an asteroid (will add it to exclusion list)
21:35:18.47 +37:59:45.7 -- not an asteroid (will add it to exclusion list)
21:44:49.77 +36:56:55.2 -- not an asteroid (will add it to exclusion list)
22:14:26.75 +39:28:50.0 -- not an asteroid (will add it to exclusion list)
22:21:28.15 +33:14:45.2 -- not an asteroid (will add it to exclusion list)
22:21:50.53 +33:31:59.9 -- not an asteroid (will add it to exclusion list)
22:18:43.00 +33:06:49.5 -- not an asteroid (will add it to exclusion list)
22:23:10.54 +33:38:55.6 -- not an asteroid (will add it to exclusion list)
22:20:27.50 +33:24:46.9 -- not an asteroid (will add it to exclusion list)
22:20:27.28 +32:54:53.0 -- not an asteroid (will add it to exclusion list)
21:47:33.56 +37:22:57.0 -- not an asteroid (will add it to exclusion list)
22:22:11.83 +33:26:57.1 -- not an asteroid (will add it to exclusion list)
22:04:23.59 +39:34:07.2 -- not an asteroid (will add it to exclusion list)
22:21:49.31 +33:27:50.1 -- not an asteroid (will add it to exclusion list)
21:23:38.46 +35:00:20.4 -- not an asteroid (will add it to exclusion list)
21:52:06.19 +38:25:44.3 -- not an asteroid (will add it to exclusion list)
21:27:12.66 +39:53:03.7 -- not an asteroid (will add it to exclusion list)
21:49:54.34 +37:45:56.2 -- not an asteroid (will add it to exclusion list)
21:31:01.72 +37:20:11.1 -- not an asteroid (will add it to exclusion list)
22:24:46.92 +33:34:08.7 -- not an asteroid (will add it to exclusion list)
22:23:13.49 +34:11:34.8 -- not an asteroid (will add it to exclusion list)
22:23:01.57 +32:47:41.3 -- not an asteroid (will add it to exclusion list)
22:23:52.56 +33:21:51.6 -- not an asteroid (will add it to exclusion list)
21:29:41.41 +38:48:31.7 -- not an asteroid (will add it to exclusion list)
21:43:31.94 +38:44:14.3 -- not an asteroid (will add it to exclusion list)
22:24:50.18 +34:08:24.7 -- not an asteroid (will add it to exclusion list)
21:22:48.69 +36:59:06.2 -- not an asteroid (will add it to exclusion list)
22:19:31.08 +33:01:21.4 -- not an asteroid (will add it to exclusion list)
22:23:11.39 +33:56:44.8 -- not an asteroid (will add it to exclusion list)
22:23:44.35 +33:36:35.5 -- not an asteroid (will add it to exclusion list)
22:23:12.06 +34:06:18.2 -- not an asteroid (will add it to exclusion list)
21:52:14.84 +36:58:30.1 -- not an asteroid (will add it to exclusion list)
22:24:04.78 +33:37:06.6 -- not an asteroid (will add it to exclusion list)
21:59:59.99 +38:42:22.6 -- not an asteroid (will add it to exclusion list)
21:14:10.55 +37:06:09.8 -- not an asteroid (will add it to exclusion list)
21:10:16.65 +40:21:13.7 -- not an asteroid (will add it to exclusion list)
22:25:23.93 +34:23:42.5 -- not an asteroid (will add it to exclusion list)
22:05:01.78 +41:27:42.7 -- not an asteroid (will add it to exclusion list)
21:16:44.70 +42:11:22.0 -- not an asteroid (will add it to exclusion list)
21:27:03.51 +35:21:31.8 -- not an asteroid (will add it to exclusion list)
21:30:44.38 +35:40:19.5 -- not an asteroid (will add it to exclusion list)
21:22:09.19 +38:06:47.4 -- not an asteroid (will add it to exclusion list)
21:12:15.77 +41:54:51.6 -- not an asteroid (will add it to exclusion list)
22:02:41.35 +37:09:20.1 -- not an asteroid (will add it to exclusion list)
21:42:10.77 +39:16:10.7 -- not an asteroid (will add it to exclusion list)
21:44:26.63 +39:22:57.4 -- not an asteroid (will add it to exclusion list)
21:48:58.48 +37:54:22.4 -- not an asteroid (will add it to exclusion list)
21:42:45.53 +38:41:54.9 -- not an asteroid (will add it to exclusion list)
22:23:06.21 +32:48:02.8 -- not an asteroid (will add it to exclusion list)
22:24:47.82 +41:23:34.6 -- not an asteroid (will add it to exclusion list)
22:14:30.42 +34:05:12.7 -- not an asteroid (will add it to exclusion list)
22:20:06.30 +33:26:31.1 -- not an asteroid (will add it to exclusion list)
21:52:37.05 +39:29:23.8 -- not an asteroid (will add it to exclusion list)
22:18:38.88 +33:13:29.2 -- not an asteroid (will add it to exclusion list)
22:22:47.01 +32:45:45.7 -- not an asteroid (will add it to exclusion list)
22:19:16.62 +33:14:56.7 -- not an asteroid (will add it to exclusion list)
22:26:22.08 +38:29:11.0 -- not an asteroid (will add it to exclusion list)
22:27:04.56 +36:34:03.6 -- not an asteroid (will add it to exclusion list)
22:25:31.35 +36:37:30.5 -- not an asteroid (will add it to exclusion list)
22:26:48.56 +40:52:45.3 -- not an asteroid (will add it to exclusion list)
22:28:59.62 +41:10:52.3 -- not an asteroid (will add it to exclusion list)
22:26:09.53 +39:20:23.0 -- not an asteroid (will add it to exclusion list)
22:23:22.75 +33:27:23.4 -- not an asteroid (will add it to exclusion list)
22:27:58.20 +41:56:15.7 -- not an asteroid (will add it to exclusion list)
22:26:35.14 +36:30:44.8 -- not an asteroid (will add it to exclusion list)
22:28:14.10 +38:59:33.1 -- not an asteroid (will add it to exclusion list)
22:27:40.80 +38:24:06.8 -- not an asteroid (will add it to exclusion list)
22:24:04.58 +41:44:25.4 -- not an asteroid (will add it to exclusion list)
22:15:55.09 +33:10:18.4 -- not an asteroid (will add it to exclusion list)
22:24:41.58 +41:00:04.8 -- not an asteroid (will add it to exclusion list)
22:20:34.56 +41:55:58.2 -- not an asteroid (will add it to exclusion list)
22:27:32.21 +40:12:34.8 -- not an asteroid (will add it to exclusion list)
22:21:24.84 +40:44:14.8 -- not an asteroid (will add it to exclusion list)
21:59:24.47 +39:22:40.2 -- not an asteroid (will add it to exclusion list)
22:18:40.15 +33:30:22.2 -- not an asteroid (will add it to exclusion list)
22:18:38.97 +33:24:05.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:10:10.05 +42:07:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:16.65 +40:21:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:17.90 +39:56:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:27.84 +36:47:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:36.29 +40:19:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:48.56 +37:16:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:15.77 +41:54:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:34.00 +38:29:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:50.82 +36:08:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:10.67 +42:30:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:10.55 +37:06:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:38.33 +37:33:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:44.97 +38:12:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:56.94 +37:19:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:17.39 +38:56:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:25.75 +36:10:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:42.98 +33:53:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:00.24 +33:40:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:44.70 +42:11:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:09.32 +42:14:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:20.43 +36:43:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:37.39 +36:35:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:44.52 +33:45:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:45.95 +35:45:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:35.27 +40:16:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:51.01 +34:56:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:48.16 +37:09:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:22.07 +36:42:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:25.16 +37:31:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:38.11 +36:33:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:52.06 +38:17:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:12.47 +36:20:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:47.69 +35:29:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:09.19 +38:06:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:36.14 +35:35:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:48.69 +36:59:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:57.41 +34:56:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:18.20 +42:11:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:28.52 +42:28:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:29.50 +39:22:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:35.23 +38:21:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:38.46 +35:00:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:39.30 +36:58:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:58.58 +36:59:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:05.62 +37:46:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:56.61 +38:11:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:13.31 +36:37:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:25.10 +35:51:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.13 +37:31:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:03.51 +35:21:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:12.66 +39:53:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:23.91 +33:39:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:28.55 +35:23:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:41.86 +38:45:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:59.75 +37:32:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:11.80 +34:45:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:04.91 +40:27:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:07.96 +42:01:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:32.56 +33:47:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:41.41 +38:48:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:44.38 +35:40:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:01.72 +37:20:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:02.09 +37:39:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.81 +38:46:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.39 +35:34:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:27.21 +38:28:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:51.75 +35:15:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:54.29 +35:30:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:55.76 +38:02:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:38.33 +37:37:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:38.97 +39:05:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:55.65 +39:39:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:28.18 +39:24:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:37.49 +34:15:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:48.59 +33:48:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:48.86 +41:16:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:00.60 +35:11:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:16.60 +37:59:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:18.47 +37:59:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:22.22 +40:35:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:54.23 +40:36:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:56.45 +40:23:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:02.81 +40:22:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:42.01 +39:56:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:40.87 +36:19:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.71 +37:23:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.21 +41:13:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:19.29 +37:02:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:29.00 +37:46:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:06.09 +36:50:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:10.77 +39:16:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:23.04 +40:36:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:45.53 +38:41:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:45.65 +36:52:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:46.24 +37:59:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:50.22 +37:29:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:55.18 +37:35:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:31.94 +38:44:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:26.63 +39:22:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:38.58 +38:02:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.77 +36:56:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:33.56 +37:22:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.05 +40:08:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:58.48 +37:54:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.34 +37:45:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.43 +34:54:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:26.30 +41:51:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:06.19 +38:25:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:08.98 +36:25:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:14.84 +36:58:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:37.05 +39:29:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:04.33 +37:39:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:57.21 +40:10:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:40.58 +37:18:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:07.65 +38:56:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:24.47 +39:22:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:27.31 +38:47:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:59.99 +38:42:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:15.54 +42:40:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:18.66 +38:06:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:54.44 +41:16:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:07.87 +39:15:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:13.39 +38:33:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:18.64 +41:30:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.40 +40:55:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:53.20 +40:17:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:40.27 +38:06:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:41.35 +37:09:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.05 +37:08:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.37 +41:44:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.94 +33:22:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.82 +39:46:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:23.59 +39:34:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:54.80 +37:38:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:01.78 +41:27:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:39.71 +34:53:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:46.39 +39:39:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:05.37 +37:55:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:49.39 +33:25:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:47.62 +38:26:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:38.32 +38:19:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:23.24 +33:35:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:26.75 +39:28:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:30.42 +34:05:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:40.29 +33:58:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:49.17 +32:48:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:55.09 +33:10:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:43.90 +33:05:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:38.58 +32:56:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:57.51 +33:00:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:05.10 +32:44:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:08.29 +32:50:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:11.58 +32:43:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:13.04 +32:48:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:18.44 +33:03:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:20.23 +32:53:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:24.32 +32:54:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:25.16 +32:55:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:32.61 +32:45:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:36.65 +32:58:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:37.77 +32:48:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:38.59 +32:52:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:38.88 +33:13:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:38.97 +33:24:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:40.15 +33:30:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:42.70 +33:05:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:43.00 +33:06:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:46.75 +32:43:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:05.13 +32:54:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:10.61 +33:01:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:12.03 +33:10:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:14.02 +32:43:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:14.40 +32:50:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:16.62 +33:14:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:18.86 +33:03:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:19.12 +32:44:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:23.14 +32:59:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:23.99 +32:46:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:26.54 +33:03:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:31.08 +33:01:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:32.53 +33:07:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:34.44 +33:14:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:37.58 +42:13:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:38.04 +33:02:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:40.49 +33:14:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:44.20 +32:47:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:44.77 +33:18:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:46.52 +33:02:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:48.19 +33:01:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:54.91 +32:47:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:05.95 +32:43:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:06.30 +33:26:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:07.11 +32:50:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:10.09 +32:56:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:18.57 +32:56:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:21.50 +32:42:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:22.16 +33:02:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:22.40 +32:56:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:23.52 +32:54:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:23.55 +33:06:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:27.28 +32:54:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:27.50 +33:24:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:28.76 +32:59:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:30.33 +32:41:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:34.56 +41:55:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:34.59 +33:02:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:37.31 +33:23:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:39.00 +32:50:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:39.20 +32:54:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:39.92 +33:27:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:40.46 +33:17:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:40.74 +33:08:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:42.31 +33:18:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:44.06 +33:02:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:45.94 +32:42:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:46.87 +32:50:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:47.78 +33:26:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:50.94 +32:53:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:55.87 +41:36:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:56.39 +32:59:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:56.51 +33:12:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:57.87 +32:46:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:01.94 +33:19:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:03.77 +33:12:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:05.10 +33:08:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:07.02 +32:55:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:07.21 +33:09:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:08.21 +33:31:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:08.78 +32:46:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:09.22 +33:14:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:11.00 +32:48:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:13.43 +32:41:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:16.32 +33:39:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:18.80 +32:47:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:20.67 +32:54:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:22.26 +32:51:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:24.84 +40:44:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:26.71 +33:33:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:27.93 +33:16:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:27.95 +33:30:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:28.15 +33:14:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:28.32 +33:30:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:28.71 +32:41:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:30.33 +33:21:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:30.45 +33:24:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:33.24 +33:09:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:33.47 +32:52:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:35.05 +32:41:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:35.28 +33:45:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:41.06 +32:47:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:41.54 +33:58:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:41.85 +33:15:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:43.44 +33:19:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:45.89 +33:23:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:46.71 +33:32:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:48.57 +33:16:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:49.31 +33:27:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:49.75 +33:05:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:50.53 +33:31:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:52.14 +33:11:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:02.85 +32:44:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:03.92 +33:34:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:07.66 +32:48:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:08.94 +33:00:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:09.47 +32:46:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:11.78 +32:41:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:11.83 +33:26:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:12.35 +33:29:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:13.07 +32:41:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:13.30 +32:50:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:16.23 +33:18:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:17.26 +32:41:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:19.37 +32:54:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:23.71 +32:51:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:24.25 +33:43:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:24.55 +33:38:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:25.23 +32:47:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:28.49 +33:46:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:28.49 +33:51:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:28.70 +33:12:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:30.21 +33:34:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:31.67 +32:40:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:33.42 +33:34:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:33.50 +33:44:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:37.60 +33:42:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:38.66 +33:28:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:39.66 +33:39:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:40.12 +33:47:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:40.25 +34:04:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:44.70 +33:19:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:47.01 +32:45:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:50.68 +33:02:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:51.88 +33:51:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:55.78 +33:33:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:56.58 +33:21:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:56.89 +33:12:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:57.67 +33:36:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:58.32 +32:58:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:59.31 +33:34:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:00.58 +33:18:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:00.98 +33:29:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:01.53 +32:54:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:01.57 +32:47:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:02.72 +32:42:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:03.75 +33:14:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:06.21 +32:48:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:07.16 +33:08:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:07.72 +33:37:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:07.90 +33:23:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:08.16 +32:50:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:10.00 +34:09:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:10.54 +33:38:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:10.70 +33:50:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:11.20 +32:49:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:11.39 +33:56:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:12.06 +34:06:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:12.48 +33:23:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:13.49 +34:11:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:15.04 +34:07:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:19.94 +33:27:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:20.66 +32:59:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:22.75 +33:27:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:22.81 +32:55:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:22.96 +33:18:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:23.41 +33:32:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:24.36 +33:31:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:25.02 +33:24:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:27.37 +33:57:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:28.06 +32:56:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:31.33 +32:43:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:33.08 +32:55:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:34.30 +33:56:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:36.58 +33:39:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:36.74 +33:59:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:37.08 +34:04:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:38.23 +33:32:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:40.39 +33:06:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:41.27 +33:35:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:42.36 +33:58:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:43.81 +33:04:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:43.93 +33:23:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:44.34 +32:54:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:44.35 +33:36:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:44.96 +32:47:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:45.42 +33:03:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:48.00 +33:17:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:48.10 +34:10:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:49.40 +33:29:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:49.51 +33:28:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:52.56 +33:21:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:52.63 +33:08:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:53.79 +32:58:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:54.63 +33:02:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:55.36 +34:07:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:55.51 +33:00:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:56.54 +33:46:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:01.94 +33:34:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:02.12 +33:51:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:02.20 +32:39:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:02.73 +34:10:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:03.21 +33:02:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:04.58 +41:44:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:04.60 +34:24:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:04.78 +33:37:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:04.84 +32:52:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:05.46 +33:35:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:06.40 +33:47:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:08.27 +33:27:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:08.92 +33:57:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:12.27 +32:53:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:13.04 +33:46:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:14.74 +33:37:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:16.55 +32:44:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:19.50 +33:47:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:19.63 +33:45:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:20.52 +34:10:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:20.54 +32:49:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:23.17 +33:12:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:26.90 +33:02:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:27.88 +33:37:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:30.17 +33:12:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:31.23 +34:22:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:35.00 +33:07:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:35.31 +33:46:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:39.03 +33:58:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:41.55 +33:06:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:41.58 +41:00:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:46.42 +33:23:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:46.92 +33:34:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:47.50 +33:40:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:47.82 +41:23:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:48.21 +34:20:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:50.18 +34:08:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:57.77 +33:32:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:04.56 +33:47:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:05.76 +34:12:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:06.51 +33:54:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:10.70 +33:50:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:19.00 +34:03:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:23.93 +34:23:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:26.04 +34:33:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:31.35 +36:37:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:35.96 +34:15:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:09.53 +39:20:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:22.08 +38:29:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:35.14 +36:30:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:48.56 +40:52:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:04.56 +36:34:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:32.21 +40:12:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:40.80 +38:24:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:58.20 +41:56:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:14.10 +38:59:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:59.62 +41:10:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:53.30 +41:26:00.2 -- 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)
21:10:10.05 +42:07:59.7 -- not a known variable star
21:10:16.65 +40:21:13.7 -- not a known variable star
21:10:17.90 +39:56:34.8 -- not a known variable star
21:10:27.84 +36:47:46.3 -- not a known variable star
21:10:36.29 +40:19:48.4 -- not a known variable star
21:11:48.56 +37:16:05.0 -- not a known variable star
21:12:15.77 +41:54:51.6 -- not a known variable star
21:12:34.00 +38:29:35.1 -- a known variable star
21:12:50.82 +36:08:09.5 -- not a known variable star
21:13:10.67 +42:30:08.0 -- a known variable star
21:14:10.55 +37:06:09.8 -- not a known variable star
21:14:38.33 +37:33:54.1 -- not a known variable star
21:14:44.97 +38:12:04.6 -- not a known variable star
21:14:56.94 +37:19:03.4 -- not a known variable star
21:15:17.39 +38:56:43.9 -- not a known variable star
21:15:25.75 +36:10:50.0 -- not a known variable star
21:15:42.98 +33:53:36.6 -- not a known variable star
21:16:00.24 +33:40:28.9 -- a known variable star
21:16:44.70 +42:11:22.0 -- not a known variable star
21:17:09.32 +42:14:59.2 -- not a known variable star
21:17:20.43 +36:43:55.1 -- not a known variable star
21:17:37.39 +36:35:15.8 -- not a known variable star
21:17:44.52 +33:45:12.7 -- not a known variable star
21:17:45.95 +35:45:18.2 -- not a known variable star
21:18:35.27 +40:16:40.9 -- not a known variable star
21:18:51.01 +34:56:41.1 -- not a known variable star
21:19:48.16 +37:09:11.9 -- not a known variable star
21:20:22.07 +36:42:26.0 -- not a known variable star
21:20:25.16 +37:31:58.3 -- not a known variable star
21:20:38.11 +36:33:48.2 -- not a known variable star
21:20:52.06 +38:17:40.1 -- not a known variable star
21:21:12.47 +36:20:38.0 -- not a known variable star
21:21:47.69 +35:29:50.1 -- not a known variable star
21:22:09.19 +38:06:47.4 -- not a known variable star
21:22:36.14 +35:35:48.6 -- not a known variable star
21:22:48.69 +36:59:06.2 -- a known variable star
21:22:57.41 +34:56:38.4 -- a known variable star
21:23:18.20 +42:11:40.3 -- not a known variable star
21:23:28.52 +42:28:11.4 -- not a known variable star
21:23:29.50 +39:22:20.0 -- not a known variable star
21:23:35.23 +38:21:42.0 -- not a known variable star
21:23:38.46 +35:00:20.4 -- not a known variable star
21:24:39.30 +36:58:43.5 -- a known variable star
21:24:58.58 +36:59:14.2 -- not a known variable star
21:25:05.62 +37:46:27.9 -- not a known variable star
21:25:56.61 +38:11:59.4 -- not a known variable star
21:26:13.31 +36:37:42.3 -- not a known variable star
21:26:25.10 +35:51:26.3 -- not a known variable star
21:26:53.13 +37:31:51.0 -- not a known variable star
21:27:03.51 +35:21:31.8 -- not a known variable star
21:27:12.66 +39:53:03.7 -- not a known variable star
21:27:23.91 +33:39:59.0 -- not a known variable star
21:27:28.55 +35:23:04.1 -- a known variable star
21:27:41.86 +38:45:47.5 -- not a known variable star
21:27:59.75 +37:32:19.5 -- not a known variable star
21:28:11.80 +34:45:27.9 -- not a known variable star
21:29:04.91 +40:27:04.7 -- not a known variable star
21:29:07.96 +42:01:04.7 -- a known variable star
21:29:32.56 +33:47:11.0 -- not a known variable star
21:29:41.41 +38:48:31.7 -- not a known variable star
21:30:44.38 +35:40:19.5 -- not a known variable star
21:31:01.72 +37:20:11.1 -- not a known variable star
21:31:02.09 +37:39:41.7 -- not a known variable star
21:31:14.81 +38:46:29.9 -- a known variable star
21:31:28.39 +35:34:31.0 -- not a known variable star
21:32:27.21 +38:28:54.9 -- not a known variable star
21:32:51.75 +35:15:27.0 -- not a known variable star
21:32:54.29 +35:30:10.2 -- not a known variable star
21:32:55.76 +38:02:35.9 -- a known variable star
21:33:38.33 +37:37:18.2 -- not a known variable star
21:33:38.97 +39:05:53.5 -- not a known variable star
21:33:55.65 +39:39:30.3 -- not a known variable star
21:34:28.18 +39:24:27.9 -- not a known variable star
21:34:37.49 +34:15:56.5 -- not a known variable star
21:34:48.59 +33:48:32.7 -- not a known variable star
21:34:48.86 +41:16:17.5 -- not a known variable star
21:35:00.60 +35:11:24.6 -- not a known variable star
21:35:16.60 +37:59:52.8 -- not a known variable star
21:35:18.47 +37:59:45.7 -- not a known variable star
21:36:22.22 +40:35:08.1 -- not a known variable star
21:36:54.23 +40:36:46.5 -- not a known variable star
21:37:56.45 +40:23:15.4 -- not a known variable star
21:39:02.81 +40:22:36.4 -- not a known variable star
21:39:42.01 +39:56:25.6 -- not a known variable star
21:40:40.87 +36:19:20.7 -- not a known variable star
21:40:43.71 +37:23:00.9 -- not a known variable star
21:40:56.21 +41:13:24.8 -- not a known variable star
21:41:19.29 +37:02:32.5 -- not a known variable star
21:41:29.00 +37:46:46.0 -- not a known variable star
21:42:06.09 +36:50:54.1 -- not a known variable star
21:42:10.77 +39:16:10.7 -- not a known variable star
21:42:23.04 +40:36:53.8 -- not a known variable star
21:42:45.53 +38:41:54.9 -- not a known variable star
21:42:45.65 +36:52:50.7 -- a known variable star
21:42:46.24 +37:59:51.7 -- not a known variable star
21:42:50.22 +37:29:33.0 -- a known variable star
21:42:55.18 +37:35:20.8 -- a known variable star
21:43:31.94 +38:44:14.3 -- not a known variable star
21:44:26.63 +39:22:57.4 -- not a known variable star
21:44:38.58 +38:02:24.8 -- not a known variable star
21:44:49.77 +36:56:55.2 -- not a known variable star
21:47:33.56 +37:22:57.0 -- not a known variable star
21:48:47.05 +40:08:13.9 -- not a known variable star
21:48:58.48 +37:54:22.4 -- not a known variable star
21:49:54.34 +37:45:56.2 -- not a known variable star
21:49:54.43 +34:54:45.8 -- not a known variable star
21:50:26.30 +41:51:43.1 -- not a known variable star
21:52:06.19 +38:25:44.3 -- not a known variable star
21:52:08.98 +36:25:24.0 -- not a known variable star
21:52:14.84 +36:58:30.1 -- not a known variable star
21:52:37.05 +39:29:23.8 -- a known variable star
21:54:04.33 +37:39:40.0 -- not a known variable star
21:55:57.21 +40:10:26.6 -- not a known variable star
21:57:40.58 +37:18:46.3 -- not a known variable star
21:58:07.65 +38:56:43.1 -- not a known variable star
21:59:24.47 +39:22:40.2 -- not a known variable star
21:59:27.31 +38:47:13.7 -- not a known variable star
21:59:59.99 +38:42:22.6 -- a known variable star
22:00:15.54 +42:40:25.6 -- not a known variable star
22:00:18.66 +38:06:30.6 -- not a known variable star
22:00:54.44 +41:16:16.1 -- not a known variable star
22:01:07.87 +39:15:18.6 -- not a known variable star
22:01:13.39 +38:33:03.0 -- not a known variable star
22:01:18.64 +41:30:28.5 -- not a known variable star
22:01:22.40 +40:55:09.3 -- not a known variable star
22:01:53.20 +40:17:20.1 -- not a known variable star
22:02:40.27 +38:06:45.8 -- not a known variable star
22:02:41.35 +37:09:20.1 -- not a known variable star
22:02:42.05 +37:08:58.3 -- not a known variable star
22:02:42.37 +41:44:11.1 -- not a known variable star
22:02:42.94 +33:22:25.8 -- not a known variable star
22:03:59.82 +39:46:39.6 -- not a known variable star
22:04:23.59 +39:34:07.2 -- not a known variable star
22:04:54.80 +37:38:40.9 -- not a known variable star
22:05:01.78 +41:27:42.7 -- not a known variable star
22:05:39.71 +34:53:40.0 -- a known variable star
22:06:46.39 +39:39:08.4 -- not a known variable star
22:07:05.37 +37:55:15.6 -- not a known variable star
22:07:49.39 +33:25:38.5 -- not a known variable star
22:11:47.62 +38:26:20.1 -- not a known variable star
22:12:38.32 +38:19:17.8 -- not a known variable star
22:13:23.24 +33:35:20.4 -- not a known variable star
22:14:26.75 +39:28:50.0 -- not a known variable star
22:14:30.42 +34:05:12.7 -- not a known variable star
22:14:40.29 +33:58:19.1 -- a known variable star
22:14:49.17 +32:48:44.8 -- not a known variable star
22:15:55.09 +33:10:18.4 -- a known variable star
22:16:43.90 +33:05:24.7 -- a known variable star
22:17:38.58 +32:56:02.4 -- not a known variable star
22:17:57.51 +33:00:25.5 -- not a known variable star
22:18:05.10 +32:44:50.7 -- not a known variable star
22:18:08.29 +32:50:45.1 -- not a known variable star
22:18:11.58 +32:43:33.2 -- not a known variable star
22:18:13.04 +32:48:49.6 -- not a known variable star
22:18:18.44 +33:03:09.3 -- not a known variable star
22:18:20.23 +32:53:58.5 -- a known variable star
22:18:24.32 +32:54:23.2 -- not a known variable star
22:18:25.16 +32:55:08.1 -- a known variable star
22:18:32.61 +32:45:57.5 -- not a known variable star
22:18:36.65 +32:58:58.0 -- not a known variable star
22:18:37.77 +32:48:16.6 -- a known variable star
22:18:38.59 +32:52:57.5 -- a known variable star
22:18:38.88 +33:13:29.2 -- not a known variable star
22:18:38.97 +33:24:05.6 -- not a known variable star
22:18:40.15 +33:30:22.2 -- not a known variable star
22:18:42.70 +33:05:54.4 -- not a known variable star
22:18:43.00 +33:06:49.5 -- a known variable star
22:18:46.75 +32:43:54.8 -- not a known variable star
22:19:05.13 +32:54:15.2 -- a known variable star
22:19:10.61 +33:01:16.8 -- not a known variable star
22:19:12.03 +33:10:14.0 -- not a known variable star
22:19:14.02 +32:43:30.4 -- not a known variable star
22:19:14.40 +32:50:53.6 -- not a known variable star
22:19:16.62 +33:14:56.7 -- not a known variable star
22:19:18.86 +33:03:23.4 -- not a known variable star
22:19:19.12 +32:44:18.3 -- not a known variable star
22:19:23.14 +32:59:21.0 -- not a known variable star
22:19:23.99 +32:46:40.9 -- not a known variable star
22:19:26.54 +33:03:40.7 -- not a known variable star
22:19:31.08 +33:01:21.4 -- not a known variable star
22:19:32.53 +33:07:17.7 -- not a known variable star
22:19:34.44 +33:14:38.1 -- not a known variable star
22:19:37.58 +42:13:56.2 -- not a known variable star
22:19:38.04 +33:02:55.3 -- not a known variable star
22:19:40.49 +33:14:50.8 -- not a known variable star
22:19:44.20 +32:47:01.0 -- not a known variable star
22:19:44.77 +33:18:41.9 -- not a known variable star
22:19:46.52 +33:02:15.5 -- not a known variable star
22:19:48.19 +33:01:21.3 -- not a known variable star
22:19:54.91 +32:47:47.2 -- not a known variable star
22:20:05.95 +32:43:47.6 -- not a known variable star
22:20:06.30 +33:26:31.1 -- not a known variable star
22:20:07.11 +32:50:48.7 -- not a known variable star
22:20:10.09 +32:56:33.4 -- not a known variable star
22:20:18.57 +32:56:13.8 -- not a known variable star
22:20:21.50 +32:42:46.3 -- not a known variable star
22:20:22.16 +33:02:14.8 -- not a known variable star
22:20:22.40 +32:56:11.9 -- not a known variable star
22:20:23.52 +32:54:15.2 -- not a known variable star
22:20:23.55 +33:06:53.7 -- not a known variable star
22:20:27.28 +32:54:53.0 -- not a known variable star
22:20:27.50 +33:24:46.9 -- a known variable star
22:20:28.76 +32:59:00.9 -- not a known variable star
22:20:30.33 +32:41:34.8 -- a known variable star
22:20:34.56 +41:55:58.2 -- not a known variable star
22:20:34.59 +33:02:40.5 -- not a known variable star
22:20:37.31 +33:23:33.2 -- a known variable star
22:20:39.00 +32:50:13.8 -- not a known variable star
22:20:39.20 +32:54:15.2 -- not a known variable star
22:20:39.92 +33:27:29.1 -- not a known variable star
22:20:40.46 +33:17:26.4 -- a known variable star
22:20:40.74 +33:08:47.3 -- not a known variable star
22:20:42.31 +33:18:15.6 -- not a known variable star
22:20:44.06 +33:02:16.2 -- not a known variable star
22:20:45.94 +32:42:31.8 -- not a known variable star
22:20:46.87 +32:50:51.1 -- not a known variable star
22:20:47.78 +33:26:03.8 -- not a known variable star
22:20:50.94 +32:53:15.3 -- not a known variable star
22:20:55.87 +41:36:26.6 -- not a known variable star
22:20:56.39 +32:59:39.1 -- not a known variable star
22:20:56.51 +33:12:56.9 -- not a known variable star
22:20:57.87 +32:46:23.1 -- not a known variable star
22:21:01.94 +33:19:23.0 -- not a known variable star
22:21:03.77 +33:12:54.3 -- not a known variable star
22:21:05.10 +33:08:35.2 -- not a known variable star
22:21:07.02 +32:55:56.2 -- not a known variable star
22:21:07.21 +33:09:50.1 -- not a known variable star
22:21:08.21 +33:31:44.5 -- not a known variable star
22:21:08.78 +32:46:19.5 -- not a known variable star
22:21:09.22 +33:14:22.0 -- not a known variable star
22:21:11.00 +32:48:09.8 -- not a known variable star
22:21:13.43 +32:41:43.0 -- not a known variable star
22:21:16.32 +33:39:10.4 -- not a known variable star
22:21:18.80 +32:47:18.4 -- not a known variable star
22:21:20.67 +32:54:29.7 -- not a known variable star
22:21:22.26 +32:51:29.8 -- not a known variable star
22:21:24.84 +40:44:14.8 -- not a known variable star
22:21:26.71 +33:33:54.4 -- not a known variable star
22:21:27.93 +33:16:36.4 -- not a known variable star
22:21:27.95 +33:30:51.2 -- a known variable star
22:21:28.15 +33:14:45.2 -- not a known variable star
22:21:28.32 +33:30:23.0 -- a known variable star
22:21:28.71 +32:41:44.2 -- not a known variable star
22:21:30.33 +33:21:21.8 -- not a known variable star
22:21:30.45 +33:24:03.5 -- a known variable star
22:21:33.24 +33:09:58.7 -- not a known variable star
22:21:33.47 +32:52:45.0 -- a known variable star
22:21:35.05 +32:41:15.4 -- not a known variable star
22:21:35.28 +33:45:23.8 -- a known variable star
22:21:41.06 +32:47:20.1 -- not a known variable star
22:21:41.54 +33:58:45.2 -- not a known variable star
22:21:41.85 +33:15:31.7 -- not a known variable star
22:21:43.44 +33:19:20.4 -- not a known variable star
22:21:45.89 +33:23:34.6 -- not a known variable star
22:21:46.71 +33:32:37.6 -- not a known variable star
22:21:48.57 +33:16:34.8 -- not a known variable star
22:21:49.31 +33:27:50.1 -- not a known variable star
22:21:49.75 +33:05:15.9 -- not a known variable star
22:21:50.53 +33:31:59.9 -- not a known variable star
22:21:52.14 +33:11:04.7 -- not a known variable star
22:22:02.85 +32:44:45.0 -- not a known variable star
22:22:03.92 +33:34:38.6 -- not a known variable star
22:22:07.66 +32:48:47.3 -- not a known variable star
22:22:08.94 +33:00:18.6 -- a known variable star
22:22:09.47 +32:46:04.4 -- not a known variable star
22:22:11.78 +32:41:01.7 -- not a known variable star
22:22:11.83 +33:26:57.1 -- not a known variable star
22:22:12.35 +33:29:02.2 -- not a known variable star
22:22:13.07 +32:41:36.1 -- not a known variable star
22:22:13.30 +32:50:51.7 -- not a known variable star
22:22:16.23 +33:18:12.1 -- not a known variable star
22:22:17.26 +32:41:43.5 -- not a known variable star
22:22:19.37 +32:54:25.7 -- not a known variable star
22:22:23.71 +32:51:01.8 -- a known variable star
22:22:24.25 +33:43:44.1 -- not a known variable star
22:22:24.55 +33:38:18.5 -- a known variable star
22:22:25.23 +32:47:16.9 -- not a known variable star
22:22:28.49 +33:46:01.3 -- a known variable star
22:22:28.49 +33:51:41.7 -- not a known variable star
22:22:28.70 +33:12:04.8 -- not a known variable star
22:22:30.21 +33:34:23.6 -- not a known variable star
22:22:31.67 +32:40:34.0 -- not a known variable star
22:22:33.42 +33:34:54.5 -- a known variable star
22:22:33.50 +33:44:26.3 -- not a known variable star
22:22:37.60 +33:42:30.3 -- not a known variable star
22:22:38.66 +33:28:06.7 -- a known variable star
22:22:39.66 +33:39:09.3 -- not a known variable star
22:22:40.12 +33:47:33.4 -- not a known variable star
22:22:40.25 +34:04:04.1 -- not a known variable star
22:22:44.70 +33:19:20.4 -- not a known variable star
22:22:47.01 +32:45:45.7 -- not a known variable star
22:22:50.68 +33:02:29.3 -- not a known variable star
22:22:51.88 +33:51:23.0 -- not a known variable star
22:22:55.78 +33:33:57.5 -- not a known variable star
22:22:56.58 +33:21:10.8 -- not a known variable star
22:22:56.89 +33:12:02.1 -- not a known variable star
22:22:57.67 +33:36:03.3 -- not a known variable star
22:22:58.32 +32:58:41.8 -- not a known variable star
22:22:59.31 +33:34:17.8 -- not a known variable star
22:23:00.58 +33:18:08.4 -- not a known variable star
22:23:00.98 +33:29:38.4 -- not a known variable star
22:23:01.53 +32:54:18.4 -- a known variable star
22:23:01.57 +32:47:41.3 -- not a known variable star
22:23:02.72 +32:42:37.5 -- not a known variable star
22:23:03.75 +33:14:11.5 -- not a known variable star
22:23:06.21 +32:48:02.8 -- not a known variable star
22:23:07.16 +33:08:02.2 -- not a known variable star
22:23:07.72 +33:37:19.1 -- not a known variable star
22:23:07.90 +33:23:02.6 -- not a known variable star
22:23:08.16 +32:50:44.2 -- not a known variable star
22:23:10.00 +34:09:20.1 -- not a known variable star
22:23:10.54 +33:38:55.6 -- not a known variable star
22:23:10.70 +33:50:35.1 -- not a known variable star
22:23:11.20 +32:49:39.7 -- not a known variable star
22:23:11.39 +33:56:44.8 -- not a known variable star
22:23:12.06 +34:06:18.2 -- not a known variable star
22:23:12.48 +33:23:24.9 -- not a known variable star
22:23:13.49 +34:11:34.8 -- not a known variable star
22:23:15.04 +34:07:35.0 -- not a known variable star
22:23:19.94 +33:27:41.0 -- not a known variable star
22:23:20.66 +32:59:09.3 -- not a known variable star
22:23:22.75 +33:27:23.4 -- not a known variable star
22:23:22.81 +32:55:55.3 -- not a known variable star
22:23:22.96 +33:18:06.0 -- not a known variable star
22:23:23.41 +33:32:22.9 -- not a known variable star
22:23:24.36 +33:31:45.1 -- not a known variable star
22:23:25.02 +33:24:37.2 -- not a known variable star
22:23:27.37 +33:57:49.6 -- not a known variable star
22:23:28.06 +32:56:28.4 -- not a known variable star
22:23:31.33 +32:43:59.5 -- a known variable star
22:23:33.08 +32:55:50.5 -- not a known variable star
22:23:34.30 +33:56:59.1 -- not a known variable star
22:23:36.58 +33:39:32.2 -- not a known variable star
22:23:36.74 +33:59:16.9 -- not a known variable star
22:23:37.08 +34:04:43.8 -- not a known variable star
22:23:38.23 +33:32:00.0 -- not a known variable star
22:23:40.39 +33:06:46.4 -- not a known variable star
22:23:41.27 +33:35:11.1 -- not a known variable star
22:23:42.36 +33:58:37.1 -- not a known variable star
22:23:43.81 +33:04:00.7 -- not a known variable star
22:23:43.93 +33:23:34.1 -- not a known variable star
22:23:44.34 +32:54:13.3 -- a known variable star
22:23:44.35 +33:36:35.5 -- not a known variable star
22:23:44.96 +32:47:18.9 -- a known variable star
22:23:45.42 +33:03:10.9 -- not a known variable star
22:23:48.00 +33:17:20.9 -- not a known variable star
22:23:48.10 +34:10:12.1 -- not a known variable star
22:23:49.40 +33:29:56.6 -- not a known variable star
22:23:49.51 +33:28:26.0 -- not a known variable star
22:23:52.56 +33:21:51.6 -- a known variable star
22:23:52.63 +33:08:36.3 -- not a known variable star
22:23:53.79 +32:58:14.7 -- not a known variable star
22:23:54.63 +33:02:50.9 -- not a known variable star
22:23:55.36 +34:07:37.3 -- not a known variable star
22:23:55.51 +33:00:55.5 -- not a known variable star
22:23:56.54 +33:46:36.7 -- not a known variable star
22:24:01.94 +33:34:40.3 -- not a known variable star
22:24:02.12 +33:51:15.8 -- not a known variable star
22:24:02.20 +32:39:09.6 -- a known variable star
22:24:02.73 +34:10:38.8 -- not a known variable star
22:24:03.21 +33:02:09.1 -- not a known variable star
22:24:04.58 +41:44:25.4 -- not a known variable star
22:24:04.60 +34:24:03.0 -- not a known variable star
22:24:04.78 +33:37:06.6 -- not a known variable star
22:24:04.84 +32:52:51.7 -- not a known variable star
22:24:05.46 +33:35:00.5 -- not a known variable star
22:24:06.40 +33:47:07.0 -- not a known variable star
22:24:08.27 +33:27:45.7 -- not a known variable star
22:24:08.92 +33:57:54.4 -- not a known variable star
22:24:12.27 +32:53:19.9 -- not a known variable star
22:24:13.04 +33:46:11.5 -- not a known variable star
22:24:14.74 +33:37:32.5 -- not a known variable star
22:24:16.55 +32:44:05.8 -- not a known variable star
22:24:19.50 +33:47:17.9 -- not a known variable star
22:24:19.63 +33:45:17.7 -- not a known variable star
22:24:20.52 +34:10:17.0 -- not a known variable star
22:24:20.54 +32:49:58.8 -- not a known variable star
22:24:23.17 +33:12:16.0 -- not a known variable star
22:24:26.90 +33:02:13.5 -- not a known variable star
22:24:27.88 +33:37:47.6 -- not a known variable star
22:24:30.17 +33:12:13.8 -- not a known variable star
22:24:31.23 +34:22:25.5 -- not a known variable star
22:24:35.00 +33:07:57.2 -- not a known variable star
22:24:35.31 +33:46:20.4 -- not a known variable star
22:24:39.03 +33:58:16.5 -- a known variable star
22:24:41.55 +33:06:45.4 -- not a known variable star
22:24:41.58 +41:00:04.8 -- not a known variable star
22:24:46.42 +33:23:51.6 -- not a known variable star
22:24:46.92 +33:34:08.7 -- a known variable star
22:24:47.50 +33:40:33.0 -- not a known variable star
22:24:47.82 +41:23:34.6 -- a known variable star
22:24:48.21 +34:20:20.0 -- not a known variable star
22:24:50.18 +34:08:24.7 -- not a known variable star
22:24:57.77 +33:32:13.7 -- not a known variable star
22:25:04.56 +33:47:39.0 -- not a known variable star
22:25:05.76 +34:12:57.2 -- not a known variable star
22:25:06.51 +33:54:39.9 -- not a known variable star
22:25:10.70 +33:50:28.1 -- a known variable star
22:25:19.00 +34:03:17.2 -- a known variable star
22:25:23.93 +34:23:42.5 -- not a known variable star
22:25:26.04 +34:33:53.2 -- not a known variable star
22:25:31.35 +36:37:30.5 -- not a known variable star
22:25:35.96 +34:15:30.1 -- not a known variable star
22:26:09.53 +39:20:23.0 -- a known variable star
22:26:22.08 +38:29:11.0 -- not a known variable star
22:26:35.14 +36:30:44.8 -- not a known variable star
22:26:48.56 +40:52:45.3 -- not a known variable star
22:27:04.56 +36:34:03.6 -- not a known variable star
22:27:32.21 +40:12:34.8 -- not a known variable star
22:27:40.80 +38:24:06.8 -- not a known variable star
22:27:58.20 +41:56:15.7 -- not a known variable star
22:28:14.10 +38:59:33.1 -- not a known variable star
22:28:59.62 +41:10:52.3 -- a known variable star
22:29:53.30 +41:26:00.2 -- not a known variable star
Found 361 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
414 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 414 (excluding asteroids and hot pixels, 361 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461179.78924895 -observatory V36
04:05:50.44 +21:48:27.9 Mercury (-1.8mag)
05:59:38.92 +25:02:27.5 Venus (-3.9mag)
01:52:19.04 +10:44:13.7 Mars (1.3mag)
07:32:47.73 +22:07:53.0 Jupiter (-1.9mag)
00:42:52.11 +02:11:49.8 Saturn (0.9mag)
03:55:23.47 +20:11:19.1 Uranus (5.8mag)
00:14:37.74 +00:08:00.2 Neptune (7.8mag)
20:34:07.61 -22:58:02.5 Pluto (14.5mag)
06:10:38.45 +27:01:22.7 Moon (-8.9mag)
-rw-r--r-- 1 apache apache 362 May 19 02:29 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461179.78924895:
07:32:41.49 +22:08:09.4 Io (5.9mag)
07:32:55.58 +22:07:30.7 Europa (6.1mag)
07:32:44.51 +22:08:07.4 Ganymede (5.5mag)
07:33:19.98 +22:06:32.2 Callisto (6.7mag)
07:34:18.23 +21:45:00.3 Himalia (15.5mag)
07:32:44.91 +22:08:01.3 Thebe (16.4mag)
07:34:43.04 +22:09:07.6 Elara (17.5mag)
07:33:50.98 +22:30:20.3 Pasiphae (17.6mag)
07:40:10.10 +22:08:17.5 Carme (18.7mag)
00:42:47.73 +02:12:19.2 Titan (8.7mag)
00:42:57.75 +02:11:49.5 Rhea (10.0mag)
00:42:59.54 +02:10:45.2 Iapetus (11.4mag)
00:42:54.23 +02:11:26.5 Hyperion (14.7mag)
00:43:57.43 +02:16:33.3 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 19 02:29 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461179.78924895:
17:09:56.24 -31:43:56.3 JWST
18:11:01.05 +32:24:30.0 Chandra
19:11:16.91 -06:01:12.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 19 02:29 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461179.78924895 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
13:27:22.86 -27:45:17.8 14.5mag D/1884 O1 (Barnard)
06:25:29.13 +30:49:38.0 15.8mag D/1886 K1 (Brooks)
15:32:39.43 +00:59:40.2 14.7mag D/1895 Q1 (Swift)
05:17:07.93 +24:22:43.0 17.1mag D/1918 W1 (Schorr)
08:41:23.22 +20:27:53.1 17.8mag P/2009 WX51 (Catalina)
18:53:41.20 -31:06:49.6 13.7mag P/2010 H2 (Vales)
05:34:26.03 -68:25:38.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:41:58.10 +31:43:52.6 17.4mag C/2017 K2 (PANSTARRS)
17:22:24.03 +14:00:30.0 17.7mag C/2021 G2 (ATLAS)
23:14:49.97 +30:43:52.8 17.2mag C/2022 E2 (ATLAS)
05:09:29.67 +26:45:48.2 16.3mag C/2022 N2 (PANSTARRS)
09:16:50.43 +31:40:20.5 16.5mag C/2022 QE78 (ATLAS)
08:40:57.20 +02:46:01.5 17.6mag C/2022 R6 (PANSTARRS)
18:40:18.34 +20:52:57.1 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:27:21.89 -11:05:16.8 17.5mag P/2023 B1 (PANSTARRS)
08:59:43.23 -07:23:26.3 18.0mag C/2023 F3 (ATLAS)
22:15:14.33 +65:10:11.9 17.7mag C/2023 H5 (Lemmon)
18:31:40.53 -05:02:07.6 13.8mag C/2023 R1 (PANSTARRS)
14:17:41.61 +87:05:47.0 17.9mag C/2023 X2 (Lemmon)
06:45:21.51 +63:46:24.0 17.5mag C/2024 A1 (ATLAS)
06:15:33.01 +25:35:18.7 12.8mag C/2024 E1 (Wierzchos)
15:53:39.72 +11:22:32.2 17.3mag C/2024 G6 (ATLAS)
20:21:57.76 +25:02:52.9 14.2mag C/2024 J3 (ATLAS)
03:58:06.96 -17:57:17.7 16.1mag C/2024 T5 (ATLAS)
05:47:07.82 +38:06:19.2 17.9mag C/2025 J1 (Borisov)
11:55:45.33 +53:25:28.2 16.7mag C/2025 L1 (ATLAS)
06:08:15.94 -09:31:27.6 11.7mag C/2025 R3 (PANSTARRS)
12:42:19.62 +04:28:58.0 17.2mag C/2025 Y1 (ATLAS)
01:22:04.07 +41:44:19.2 15.6mag C/2026 B2 (Sun-Gao)
11:11:37.36 -12:20:05.3 16.2mag A/2026 E1
19:46:46.28 -08:11:09.0 9.9mag 10P/Tempel
14:22:37.41 -01:27:42.2 17.0mag 24P/Schaumasse
10:59:08.33 -00:52:35.8 15.9mag 29P/Schwassmann-Wachmann
10:47:03.98 -02:35:51.8 17.6mag 43P/Wolf-Harrington
02:40:40.26 +22:49:30.3 17.5mag 47P/Ashbrook-Jackson
08:17:38.72 +29:10:45.3 16.9mag 63P/Wild
00:07:52.76 -07:54:52.1 15.7mag 65P/Gunn
05:39:59.14 +30:25:05.5 16.4mag 76P/West-Kohoutek-Ikemura
02:21:39.09 +14:18:11.9 14.0mag 78P/Gehrels
00:34:25.46 +00:04:03.0 15.2mag 88P/Howell
03:50:48.85 +27:55:50.2 15.1mag 93P/Lovas
06:04:16.03 +33:20:08.5 15.8mag 123P/West-Hartley
09:16:34.04 +23:17:54.1 16.4mag 124P/Mrkos
03:26:19.03 +17:42:40.6 16.4mag 128P/Shoemaker-Holt
03:53:45.68 +17:50:58.7 17.7mag 131P/Mueller
04:24:21.29 +19:39:14.0 12.2mag 141P/Machholz
04:27:33.47 +15:10:20.1 12.1mag 141P-A/Machholz
03:09:46.19 +11:55:08.2 10.5mag 141P-D/Machholz
02:43:00.50 -27:48:20.8 17.5mag 161P/Hartley-IRAS
02:38:41.30 +15:02:14.2 14.8mag 162P/SidingSpring
19:31:51.64 -03:16:16.5 17.9mag 169P/NEAT
17:07:24.03 -10:00:07.9 16.2mag 235P/LINEAR
06:49:15.24 +35:55:15.3 17.3mag 240P/NEAT
23:40:53.10 -10:23:08.6 16.9mag 260P/McNaught
03:12:47.06 +28:26:04.7 17.7mag 295P/LINEAR
20:52:25.90 -34:47:42.2 18.0mag 320P/McNaught
15:25:33.21 +08:20:53.2 17.4mag 391P/Kowalski
07:52:21.86 +21:09:25.4 17.8mag 450P/LONEOS
06:27:34.96 +43:02:02.4 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 3.0K May 19 02:29 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 19 02:29 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 19 02:29 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:42:13.520 -12:30:36.22 AT 2026mio 2026-05-11.36 20.1
11:29:43.852 +79:01:05.40 AT 2026min 2026-05-12.31 18.119
23:07:06.188 -28:36:45.66 SN 2026mim 2026-05-12.38 17.669
09:07:42.745 +48:49:44.41 AT 2026mil 2026-05-12.25 19.23
00:16:38.698 -23:54:18.80 AT 2026mik 2026-05-12.41 18.045
08:39:19.980 +74:55:20.52 AT 2026mij 2026-05-12.24 18.42
16:20:03.992 +04:00:39.88 AT 2026mii 2026-05-10.42 20.5436
16:22:27.699 +09:35:03.21 AT 2026mih 2026-05-08.39 20.6508
19:47:19.801 -12:12:53.03 AT 2026mig 2026-05-09.41 20.0731
18:05:29.328 +47:13:17.03 AT 2026mif 2026-05-12.37 18.6694
20:56:06.075 -03:52:50.22 AT 2026mie 2026-05-11.45 19.8533
20:29:21.696 -11:25:37.62 AT 2026mid 2026-05-11.45 19.5368
22:59:55.085 +16:56:56.27 AT 2026mic 2026-05-09.48 19.9296
00:29:36.385 +27:22:41.46 AT 2026mib 2026-05-09.49 19.283
16:09:40.707 -21:30:40.88 AT 2026mia 2026-04-15.46 20.4494
10:43:27.294 +20:46:08.47 AT 2026mhz 2026-02-07.38 20.217
15:37:36.960 +02:16:24.20 AT 2026mhy 2026-04-24.43 20.6382
14:15:34.017 -22:43:04.24 AT 2026mhx 2026-04-23.38 20.2188
15:22:29.741 -26:23:50.21 AT 2026mhw 2026-05-08.36 20.2311
13:34:55.030 -00:25:52.51 AT 2026mhv 2026-05-10.25 19.1402
-rw-r--r-- 1 apache apache 30K May 19 02:29 tns_transients_list.txt
