This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.49 00:19:57.42 +31:28:54.4
115.10929 -30.91134 galactic And Second-epoch detections are separated by 1.1" and 6.4 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 | 00:19:57.42 +31:28:54.4 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.029 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:57.42 +31:28:54.4: 13.38 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:57.42 +31:28:54.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 57.42 +31 28 54.4 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.49,0.05,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 20260710.3403 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.72 23:45:07.75 +26:50:58.3
105.11193 -33.71729 galactic Peg Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:45:07.75 +26:50:58.3 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.691+/-0.031 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:45:07.75 +26:50:58.3: 13.59 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:45:07.75 +26:50:58.3: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.72,0.05,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 20260710.3403 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.75 00:22:13.77 +32:01:34.7
115.75220 -30.43792 galactic And Second-epoch detections are separated by 3.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:13.77 +32:01:34.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.318+/-0.032 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:22:13.77 +32:01:34.7: 13.61 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:22:13.77 +32:01:34.7: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 22 13.77 +32 01 34.7 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.75,0.05,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 20260710.3403 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.71 23:40:55.12 +26:08:06.5
103.76324 -34.09807 galactic Peg Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:40:55.12 +26:08:06.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.701+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:40:55.12 +26:08:06.5: 13.64 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:40:55.12 +26:08:06.5: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.71,0.05,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 20260710.3403 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.68 00:20:07.89 +32:15:37.5
115.27941 -30.14572 galactic And Second-epoch detections are separated by 2.6" and 6.7 pix
The object was found in VSX10" Gaia DR3 2863307228542059392
Type: ROT
# Max. Min./Amp. JD0 Period
14.400 G 14.430 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:20:07.89 +32:15:37.5: 13.65 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:20:07.89 +32:15:37.5: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 20 07.89 +32 15 37.5 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863307228542059392,2461231.8403,12.68,0.05,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 2863307228542059392 20260710.3403 12.68CV 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 07 10.3403 2461231.8403 12.45 00:19:22.68 +30:52:09.5
114.86303 -31.49964 galactic And Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:22.68 +30:52:09.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.412+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:22.68 +30:52:09.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:22.68 +30:52:09.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 22.68 +30 52 09.5 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.45,0.05,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 20260710.3403 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.96 23:58:27.90 +33:39:51.6
110.47010 -27.92230 galactic And Second-epoch detections are separated by 3.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2875087258683610624 | 23:58:30.54 +33:40:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.662+/-0.027 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:58:27.90 +33:39:51.6: 13.88 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:58:27.90 +33:39:51.6: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 23 58 27.90 +33 39 51.6 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2875087258683610624,2461231.8403,12.96,0.05,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 2875087258683610624 20260710.3403 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.07 23:38:20.07 +27:15:17.9
103.55127 -32.85072 galactic Peg Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:20.07 +27:15:17.9 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.034 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:38:20.07 +27:15:17.9: 14.05 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:38:20.07 +27:15:17.9: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461231.8403,13.07,0.05,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 20260710.3403 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.67 00:06:14.69 +32:02:23.4
111.89164 -29.86122 galactic And Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:06:14.69 +32:02:23.4 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.031 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:14.69 +32:02:23.4: 13.52 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:06:14.69 +32:02:23.4: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 06 14.69 +32 02 23.4 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.67,0.05,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 20260710.3403 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.61 00:18:23.07 +31:52:23.4
114.79046 -30.47552 galactic And Second-epoch detections are separated by 1.5" and 6.3 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 | 00:18:23.07 +31:52:23.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.475+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:23.07 +31:52:23.4: 13.56 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:23.07 +31:52:23.4: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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!
TCP 2026 07 10.3403* 00 18 23.07 +31 52 23.4 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.61,0.05,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 20260710.3403 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.06 23:48:29.54 +26:05:23.8
105.70520 -34.66736 galactic Peg Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:48:29.54 +26:05:23.8 (user input) | T | P | (position from user input) J-Ks=0.495+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:48:29.54 +26:05:23.8: 14.05 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:48:29.54 +26:05:23.8: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 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
target,2461231.8403,13.06,0.05,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
target 20260710.3403 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.57 00:18:22.88 +32:01:36.7
114.81611 -30.32342 galactic And Second-epoch detections are separated by 0.4" and 6.3 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 | 00:18:22.88 +32:01:36.7 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:22.88 +32:01:36.7: 13.59 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:22.88 +32:01:36.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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!
TCP 2026 07 10.3403* 00 18 22.88 +32 01 36.7 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.57,0.05,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 20260710.3403 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.93 00:20:17.17 +29:02:52.8
114.78090 -33.33023 galactic And Second-epoch detections are separated by 0.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:17.17 +29:02:52.8 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.028 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:20:17.17 +29:02:52.8: 13.99 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:20:17.17 +29:02:52.8: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 20 17.17 +29 02 52.8 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.93,0.05,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 20260710.3403 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.92 00:18:52.81 +31:26:00.4
114.83628 -30.92599 galactic And Second-epoch detections are separated by 1.6" and 6.4 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 | 00:18:52.81 +31:26:00.4 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:52.81 +31:26:00.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:52.81 +31:26:00.4: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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!
TCP 2026 07 10.3403* 00 18 52.81 +31 26 00.4 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.93 00:18:36.04 +31:48:09.3
114.83104 -30.55212 galactic And Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:36.04 +31:48:09.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.417+/-0.031 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:36.04 +31:48:09.3: 13.87 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:36.04 +31:48:09.3: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 36.04 +31 48 09.3 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.93,0.05,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 20260710.3403 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.80 00:18:37.99 +32:00:41.1
114.87464 -30.34658 galactic And Second-epoch detections are separated by 0.9" and 6.4 pix
The object was found in VSX 1" Gaia DR3 2863211845908230016
Type: ROT
# Max. Min./Amp. JD0 Period
13.610 G 13.630 G 14.658700000000 K
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:37.99 +32:00:41.1: 13.87 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:37.99 +32:00:41.1: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 37.99 +32 00 41.1 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863211845908230016,2461231.8403,12.80,0.05,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 2863211845908230016 20260710.3403 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.86 00:17:27.85 +31:48:25.1
114.55464 -30.51154 galactic And Second-epoch detections are separated by 1.6" and 6.2 pix
The object was found in VSX 8" Gaia DR3 2863179994430719232
Type: E
# Max. Min./Amp. JD0 Period
16.250 G 16.720 G 0.288488000000 M
ATTENTION: measured mag 12.86 is 3.4 mag brighter than the VSX record maximum brightness 16.25 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:17:27.85 +31:48:25.1: 13.86 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:17:27.85 +31:48:25.1: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 17 27.85 +31 48 25.1 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863179994430719232,2461231.8403,12.86,0.05,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
Gaia DR3 2863179994430719232 20260710.3403 12.86CV 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 07 10.3403 2461231.8403 13.09 23:47:26.38 +27:13:25.2
105.83601 -33.51458 galactic Peg Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:47:26.38 +27:13:25.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.392+/-0.032 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:26.38 +27:13:25.2: 14.02 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:47:26.38 +27:13:25.2: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.13 00:19:14.36 +32:03:51.1
115.03080 -30.31309 galactic And Second-epoch detections are separated by 1.1" and 6.3 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 | 00:19:14.36 +32:03:51.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.344+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:14.36 +32:03:51.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:14.36 +32:03:51.1: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 14.36 +32 03 51.1 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.13,0.05,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 20260710.3403 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.63 23:37:39.46 +27:28:03.3
103.46706 -32.60019 galactic Peg Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:37:39.46 +27:28:03.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:37:39.46 +27:28:03.3: 13.50 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:37:39.46 +27:28:03.3: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.63,0.05,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 20260710.3403 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.61 00:19:24.16 +29:17:59.7
114.59691 -33.05283 galactic And Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:24.16 +29:17:59.7 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.032 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:24.16 +29:17:59.7: 13.53 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:24.16 +29:17:59.7: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 24.16 +29 17 59.7 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.61,0.05,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 20260710.3403 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.71 23:46:26.30 +26:19:49.2
105.25835 -34.30081 galactic Peg Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:46:26.30 +26:19:49.2 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:46:26.30 +26:19:49.2: 13.50 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:46:26.30 +26:19:49.2: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.71,0.05,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 20260710.3403 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.01 23:39:33.17 +26:53:45.2
103.71517 -33.27924 galactic Peg Second-epoch detections are separated by 2.0" and 6.4 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 | 23:39:33.17 +26:53:45.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.475+/-0.032 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:39:33.17 +26:53:45.2: 13.98 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:39:33.17 +26:53:45.2: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.68 23:44:51.60 +27:30:37.7
105.28488 -33.06954 galactic Peg Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:51.60 +27:30:37.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.386+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:44:51.60 +27:30:37.7: 13.73 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:44:51.60 +27:30:37.7: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.68,0.05,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 20260710.3403 12.68CV 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 07 10.3403 2461231.8403 12.93 23:48:46.52 +26:53:07.3
106.05923 -33.92496 galactic Peg Second-epoch detections are separated by 2.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:48:46.52 +26:53:07.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.344+/-0.032 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:48:46.52 +26:53:07.3: 13.98 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:48:46.52 +26:53:07.3: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.93,0.05,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 20260710.3403 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.97 00:17:07.99 +31:33:49.7
114.43041 -30.74102 galactic And Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:07.99 +31:33:49.7 (user input) | T | P | (position from user input) J-Ks=0.702+/-0.031 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:17:07.99 +31:33:49.7: 14.00 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:17:07.99 +31:33:49.7: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 17 07.99 +31 33 49.7 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.97,0.05,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 20260710.3403 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.12 23:45:11.33 +27:31:15.2
105.37156 -33.08175 galactic Peg Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:45:11.33 +27:31:15.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.431+/-0.031 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:45:11.33 +27:31:15.2: 14.14 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:45:11.33 +27:31:15.2: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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
target,2461231.8403,13.12,0.05,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 20260710.3403 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.99 23:38:59.82 +27:45:30.3
103.91322 -32.42395 galactic Peg Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:59.82 +27:45:30.3 (user input) | T | P | (position from user input) J-Ks=0.543+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:38:59.82 +27:45:30.3: 13.86 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:38:59.82 +27:45:30.3: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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
target,2461231.8403,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.05 23:39:16.36 +27:01:48.4
103.69745 -33.13195 galactic Peg Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:16.36 +27:01:48.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:39:16.36 +27:01:48.4: 14.15 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:39:16.36 +27:01:48.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461231.8403,13.05,0.05,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
target 20260710.3403 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.83 00:19:27.51 +29:17:12.2
114.60895 -33.06768 galactic And Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:27.51 +29:17:12.2 (user input) | T | P | (position from user input) J-Ks=0.842+/-0.030 (M)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:27.51 +29:17:12.2: 13.88 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:27.51 +29:17:12.2: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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!
TCP 2026 07 10.3403* 00 19 27.51 +29 17 12.2 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.83,0.05,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 20260710.3403 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.70 23:48:18.33 +26:34:42.3
105.83023 -34.18807 galactic Peg Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:48:18.33 +26:34:42.3 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.029 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:48:18.33 +26:34:42.3: 13.49 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:48:18.33 +26:34:42.3: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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
target,2461231.8403,12.70,0.05,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 20260710.3403 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.22 23:50:54.35 +26:59:36.3
106.64497 -33.95665 galactic Peg Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:50:54.35 +26:59:36.3 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:50:54.35 +26:59:36.3: 14.31 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:50:54.35 +26:59:36.3: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,13.22,0.05,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 20260710.3403 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.80 23:44:47.18 +27:37:17.5
105.30662 -32.95879 galactic Peg Second-epoch detections are separated by 2.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:47.18 +27:37:17.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.458+/-0.029 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:44:47.18 +27:37:17.5: 13.71 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:44:47.18 +27:37:17.5: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.80,0.05,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
target 20260710.3403 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.74 23:59:13.86 +28:35:05.4
109.27082 -32.89822 galactic Peg Second-epoch detections are separated by 2.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:59:13.86 +28:35:05.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.447+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:59:13.86 +28:35:05.4: 13.72 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:59:13.86 +28:35:05.4: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.74,0.05,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 20260710.3403 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.43 00:18:56.27 +31:48:54.1
114.91544 -30.55032 galactic And Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:56.27 +31:48:54.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.422+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:56.27 +31:48:54.1: 13.31 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:56.27 +31:48:54.1: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 56.27 +31 48 54.1 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.43,0.05,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
target 20260710.3403 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.91 23:47:11.10 +27:01:31.2
105.70074 -33.68736 galactic Peg Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:47:11.10 +27:01:31.2 (user input) | T | P | (position from user input) J-Ks=0.663+/-0.029 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:11.10 +27:01:31.2: 13.86 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:47:11.10 +27:01:31.2: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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
target,2461231.8403,12.91,0.05,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 20260710.3403 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.12 00:17:58.10 +33:06:48.7
114.90265 -29.23587 galactic And Second-epoch detections are separated by 0.3" and 6.3 pix
The object was found in VSX 2" Gaia DR3 2863596881136572544
Type: ROT
# Max. Min./Amp. JD0 Period
12.520 G 12.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:17:58.10 +33:06:48.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:17:58.10 +33:06:48.7: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 17 58.10 +33 06 48.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863596881136572544,2461231.8403,12.12,0.05,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 2863596881136572544 20260710.3403 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.57 23:37:10.23 +27:28:14.2
103.34745 -32.56111 galactic Peg Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:37:10.23 +27:28:14.2 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:37:10.23 +27:28:14.2: 13.46 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:37:10.23 +27:28:14.2: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 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,2461231.8403,12.57,0.05,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 20260710.3403 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.85 23:49:10.92 +27:14:47.4
106.28870 -33.60523 galactic Peg Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:49:10.92 +27:14:47.4 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.031 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:49:10.92 +27:14:47.4: 13.82 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:49:10.92 +27:14:47.4: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.85,0.05,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 20260710.3403 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.74 00:21:04.14 +31:10:04.9
115.33264 -31.25521 galactic And Second-epoch detections are separated by 3.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:04.14 +31:10:04.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:21:04.14 +31:10:04.9: 13.68 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:21:04.14 +31:10:04.9: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 21 04.14 +31 10 04.9 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.74,0.05,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 20260710.3403 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.73 00:18:40.56 +32:46:11.7
115.01321 -29.59758 galactic And Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:40.56 +32:46:11.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.670+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:40.56 +32:46:11.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:40.56 +32:46:11.7: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 40.56 +32 46 11.7 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.73,0.05,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 20260710.3403 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.98 23:53:02.20 +27:21:59.7
107.31706 -33.72815 galactic Peg Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.2575+27.3655 | 23:53:02.20 +27:21:59.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:53:02.20 +27:21:59.7: 13.98 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:53:02.20 +27:21:59.7: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 J358.2575+27.3655,2461231.8403,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.2575+27.3655 20260710.3403 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.30 23:38:54.11 +26:55:49.7
103.56500 -33.19873 galactic Peg Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:54.11 +26:55:49.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.610+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:38:54.11 +26:55:49.7: 13.25 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:38:54.11 +26:55:49.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.36 00:18:56.27 +32:25:42.5
115.01884 -29.94342 galactic And Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:56.27 +32:25:42.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.292+/-0.028 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:56.27 +32:25:42.5: 13.23 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:56.27 +32:25:42.5: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 56.27 +32 25 42.5 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.36,0.05,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 20260710.3403 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.72 00:19:01.13 +31:51:06.7
114.94143 -30.51639 galactic And Second-epoch detections are separated by 0.8" and 6.3 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 | 00:19:01.13 +31:51:06.7 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.397+/-0.029 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:01.13 +31:51:06.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:01.13 +31:51:06.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 01.13 +31 51 06.7 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.72,0.05,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 20260710.3403 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.89 23:48:01.39 +26:27:20.0
105.71359 -34.28699 galactic Peg Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:48:01.39 +26:27:20.0 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:48:01.39 +26:27:20.0: 13.85 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:48:01.39 +26:27:20.0: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461231.8403,12.89,0.05,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 20260710.3403 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.05 00:06:04.71 +31:59:37.2
111.84108 -29.89934 galactic Peg Second-epoch detections are separated by 0.3" and 6.3 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 | 00:06:04.71 +31:59:37.2 (user input) | T | P | (position from user input) J-Ks=0.232+/-0.038 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:04.71 +31:59:37.2: 13.95 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:06:04.71 +31:59:37.2: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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
target,2461231.8403,13.05,0.05,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
target 20260710.3403 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.79 00:22:47.21 +31:48:29.2
115.85540 -30.66965 galactic And Second-epoch detections are separated by 1.4" and 6.4 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 | 00:22:47.21 +31:48:29.2 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.412+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:22:47.21 +31:48:29.2: 13.68 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:22:47.21 +31:48:29.2: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 22 47.21 +31 48 29.2 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.79,0.05,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 20260710.3403 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.87 00:13:55.62 +34:27:47.7
114.19871 -27.77160 galactic And Second-epoch detections are separated by 1.4" and 6.3 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 | 00:13:55.62 +34:27:47.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.275+/-0.032 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:13:55.62 +34:27:47.7: 13.83 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:13:55.62 +34:27:47.7: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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!
TCP 2026 07 10.3403* 00 13 55.62 +34 27 47.7 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.87,0.05,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 20260710.3403 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.88 00:03:21.66 +33:50:35.9
111.63844 -27.97193 galactic And Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:03:21.66 +33:50:35.9 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.034 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:03:21.66 +33:50:35.9: 13.81 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:03:21.66 +33:50:35.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 03 21.66 +33 50 35.9 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.88,0.05,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 20260710.3403 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.82 23:45:14.18 +27:19:31.9
105.31284 -33.27112 galactic Peg Second-epoch detections are separated by 2.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:45:14.18 +27:19:31.9 (user input) | T | P | (position from user input) SpType: M2 (LAMOST DR5) J-Ks=0.856+/-0.030 (M)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:45:14.18 +27:19:31.9: 13.82 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:45:14.18 +27:19:31.9: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.82,0.05,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 20260710.3403 12.82CV 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 07 10.3403 2461231.8403 12.87 23:44:04.35 +27:45:46.2
105.17885 -32.77597 galactic Peg Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:04.35 +27:45:46.2 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:44:04.35 +27:45:46.2: 13.79 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:44:04.35 +27:45:46.2: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.87,0.05,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 20260710.3403 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.86 23:39:46.00 +26:36:10.2
103.65383 -33.57171 galactic Peg Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:46.00 +26:36:10.2 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:39:46.00 +26:36:10.2: 13.80 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:39:46.00 +26:36:10.2: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461231.8403,12.86,0.05,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 20260710.3403 12.86CV 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 07 10.3403 2461231.8403 12.77 00:20:20.53 +29:09:06.8
114.81329 -33.22919 galactic And Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:20.53 +29:09:06.8 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.026 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:20:20.53 +29:09:06.8: 13.65 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:20:20.53 +29:09:06.8: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 20 20.53 +29 09 06.8 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.77,0.05,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 20260710.3403 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.85 00:03:33.93 +32:03:16.4
111.25504 -29.72941 galactic And Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:03:33.93 +32:03:16.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.374+/-0.037 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:03:33.93 +32:03:16.4: 13.78 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:03:33.93 +32:03:16.4: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 03 33.93 +32 03 16.4 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.85,0.05,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 20260710.3403 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.06 23:40:04.98 +26:41:09.5
103.76666 -33.51634 galactic Peg Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:40:04.98 +26:41:09.5 (user input) | T | P | (position from user input) J-Ks=0.550+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:40:04.98 +26:41:09.5: 14.13 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:40:04.98 +26:41:09.5: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461231.8403,13.06,0.05,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
target 20260710.3403 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.84 23:37:59.61 +27:11:22.5
103.44024 -32.88713 galactic Peg Second-epoch detections are separated by 2.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:37:59.61 +27:11:22.5 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:37:59.61 +27:11:22.5: 13.79 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:37:59.61 +27:11:22.5: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461231.8403,12.84,0.05,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 20260710.3403 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.62 00:19:14.58 +31:59:26.0
115.01936 -30.38607 galactic And Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:14.58 +31:59:26.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.350+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:14.58 +31:59:26.0: 13.61 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:14.58 +31:59:26.0: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 14.58 +31 59 26.0 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.62,0.05,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 20260710.3403 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.73 23:44:21.56 +27:26:31.3
105.13373 -33.10081 galactic Peg Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:21.56 +27:26:31.3 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.499+/-0.025 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:44:21.56 +27:26:31.3: 13.64 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:44:21.56 +27:26:31.3: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.73,0.05,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 20260710.3403 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.91 23:39:08.12 +27:45:51.7
103.94979 -32.42836 galactic Peg Second-epoch detections are separated by 2.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:08.12 +27:45:51.7 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:39:08.12 +27:45:51.7: 13.94 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:39:08.12 +27:45:51.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461231.8403,12.91,0.05,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 20260710.3403 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.91 23:39:27.28 +26:52:12.5
103.68032 -33.29636 galactic Peg Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:27.28 +26:52:12.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.409+/-0.028 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:39:27.28 +26:52:12.5: 13.78 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:39:27.28 +26:52:12.5: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.91,0.05,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 20260710.3403 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.98 23:36:18.93 +27:47:00.4
103.26134 -32.20272 galactic Peg Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:36:18.93 +27:47:00.4 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:36:18.93 +27:47:00.4: 13.94 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:36:18.93 +27:47:00.4: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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
target,2461231.8403,12.98,0.05,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 20260710.3403 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.72 23:44:15.99 +27:27:38.4
105.11715 -33.07675 galactic Peg Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:15.99 +27:27:38.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.457+/-0.026 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:44:15.99 +27:27:38.4: 13.64 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:44:15.99 +27:27:38.4: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.72,0.05,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 20260710.3403 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.71 23:38:30.96 +27:18:04.2
103.61479 -32.82052 galactic Peg Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:30.96 +27:18:04.2 (user input) | T | P | (position from user input) J-Ks=0.725+/-0.033 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:38:30.96 +27:18:04.2: 13.63 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:38:30.96 +27:18:04.2: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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
target,2461231.8403,12.71,0.05,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 20260710.3403 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.71 23:47:46.97 +27:23:36.1
105.98298 -33.37470 galactic Peg Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:47:46.97 +27:23:36.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.340+/-0.031 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:46.97 +27:23:36.1: 13.60 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:47:46.97 +27:23:36.1: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.71,0.05,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 20260710.3403 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.71 00:16:42.66 +31:25:02.5
114.30039 -30.87169 galactic And Second-epoch detections are separated by 1.5" and 6.4 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 | 00:16:42.66 +31:25:02.5 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.235+/-0.034 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:16:42.66 +31:25:02.5: 13.62 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:16:42.66 +31:25:02.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 16 42.66 +31 25 02.5 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.71,0.05,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 20260710.3403 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.47 00:17:49.65 +33:02:03.5
114.85569 -29.30982 galactic And Second-epoch detections are separated by 0.8" and 6.4 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 | 00:17:49.65 +33:02:03.5 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.036 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:17:49.65 +33:02:03.5: 13.39 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:17:49.65 +33:02:03.5: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 17 49.65 +33 02 03.5 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.47,0.05,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 20260710.3403 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.66 00:19:51.38 +31:33:56.6
115.09846 -30.82520 galactic And Second-epoch detections are separated by 0.5" and 6.4 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 | 00:19:51.38 +31:33:56.6 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.034 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:51.38 +31:33:56.6: 13.61 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:51.38 +31:33:56.6: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 51.38 +31 33 56.6 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.93 23:36:47.87 +27:49:40.5
103.39773 -32.19686 galactic Peg Second-epoch detections are separated by 2.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:36:47.87 +27:49:40.5 (user input) | T | P | (position from user input) J-Ks=0.813+/-0.025 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:36:47.87 +27:49:40.5: 13.91 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:36:47.87 +27:49:40.5: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461231.8403,12.93,0.05,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 20260710.3403 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.88 23:45:36.36 +26:28:02.6
105.09379 -34.11372 galactic Peg Second-epoch detections are separated by 2.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.4014+26.4673 | 23:45:36.36 +26:28:02.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.664+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:45:36.36 +26:28:02.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:45:36.36 +26:28:02.6: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.4014+26.4673,2461231.8403,12.88,0.05,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 J356.4014+26.4673 20260710.3403 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.01 23:46:11.31 +26:43:31.0
105.33772 -33.90738 galactic Peg Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:46:11.31 +26:43:31.0 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.616+/-0.030 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:46:11.31 +26:43:31.0: 14.06 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:46:11.31 +26:43:31.0: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.80 00:18:40.31 +29:08:53.9
114.38157 -33.17886 galactic And Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:40.31 +29:08:53.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.540+/-0.033 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:40.31 +29:08:53.9: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:40.31 +29:08:53.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 40.31 +29 08 53.9 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.80,0.05,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
target 20260710.3403 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.79 23:43:48.31 +27:06:29.2
104.87060 -33.38051 galactic Peg Second-epoch detections are separated by 1.0" and 7.0 pix
The object was found in VSX 1" NSVS 6272051
Type: EA
# Max. Min./Amp. JD0 Period
13.660 R1 Y 1.320 R1 2.158093660000
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:43:48.31 +27:06:29.2: 13.76 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:43:48.31 +27:06:29.2: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 6272051,2461231.8403,12.79,0.05,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
NSVS 6272051 20260710.3403 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.02 00:05:18.44 +32:46:56.2
111.84162 -29.09410 galactic And Second-epoch detections are separated by 3.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:05:18.44 +32:46:56.2 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.614+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:05:18.44 +32:46:56.2: 14.07 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:05:18.44 +32:46:56.2: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.05 +/- 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!
TCP 2026 07 10.3403* 00 05 18.44 +32 46 56.2 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,13.02,0.05,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 20260710.3403 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.89 00:19:37.88 +30:36:32.9
114.88193 -31.76496 galactic And Second-epoch detections are separated by 1.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:37.88 +30:36:32.9 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.033 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:37.88 +30:36:32.9: 14.07 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:37.88 +30:36:32.9: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 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!
TCP 2026 07 10.3403* 00 19 37.88 +30 36 32.9 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.89,0.05,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 20260710.3403 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.46 23:37:59.10 +27:25:35.2
103.53206 -32.66320 galactic Peg Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:37:59.10 +27:25:35.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.369+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:37:59.10 +27:25:35.2: 13.34 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:37:59.10 +27:25:35.2: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.46,0.05,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 20260710.3403 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.92 23:49:26.26 +27:08:30.7
106.31814 -33.72177 galactic Peg Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:49:26.26 +27:08:30.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.451+/-0.028 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:49:26.26 +27:08:30.7: 13.91 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:49:26.26 +27:08:30.7: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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
target,2461231.8403,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3403 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 13.02 00:18:36.10 +29:10:50.3
114.36935 -33.14458 galactic And Second-epoch detections are separated by 2.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:36.10 +29:10:50.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.350+/-0.037 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:36.10 +29:10:50.3: 14.20 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:36.10 +29:10:50.3: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
TCP 2026 07 10.3403* 00 18 36.10 +29 10 50.3 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,13.02,0.05,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 20260710.3403 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.60 00:19:50.15 +32:06:59.5
115.18428 -30.27936 galactic And Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:50.15 +32:06:59.5 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.037 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:50.15 +32:06:59.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:50.15 +32:06:59.5: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 50.15 +32 06 59.5 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.60,0.05,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 20260710.3403 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.15 00:19:00.70 +32:04:08.7
114.97634 -30.30126 galactic And Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:00.70 +32:04:08.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.513+/-0.028 (K)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:00.70 +32:04:08.7: 13.12 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:00.70 +32:04:08.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 00.70 +32 04 08.7 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.15,0.05,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 20260710.3403 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.64 00:19:23.20 +29:21:22.9
114.60275 -32.99649 galactic And Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:23.20 +29:21:22.9 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.034 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:23.20 +29:21:22.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:23.20 +29:21:22.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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!
TCP 2026 07 10.3403* 00 19 23.20 +29 21 22.9 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.64,0.05,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
target 20260710.3403 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.75 00:18:07.64 +31:07:18.4
114.59643 -31.21026 galactic And Second-epoch detections are separated by 1.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:07.64 +31:07:18.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.382+/-0.030 (G)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:18:07.64 +31:07:18.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:18:07.64 +31:07:18.4: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 18 07.64 +31 07 18.4 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.75,0.05,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 20260710.3403 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.71 00:19:42.87 +29:18:24.5
114.67834 -33.05603 galactic And Second-epoch detections are separated by 0.3" and 6.6 pix
The object was found in VSX 1" ASASSN-V J001942.91+291824.8
Type: ROT
# Max. Min./Amp. JD0 Period
14.320 g Y 0.250 g 2459174.56100 4.524600000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:19:42.87 +29:18:24.5: 13.75 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:19:42.87 +29:18:24.5: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 19 42.87 +29 18 24.5 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J001942.91+291824.8,2461231.8403,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J001942.91+291824.8 20260710.3403 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.83 00:14:37.47 +32:15:21.9
113.94917 -29.97274 galactic And Second-epoch detections are separated by 0.4" and 6.3 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 | 00:14:37.47 +32:15:21.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.303+/-0.058 (F)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:14:37.47 +32:15:21.9: 13.75 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:14:37.47 +32:15:21.9: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3403* 00 14 37.47 +32 15 21.9 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8403,12.83,0.05,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 20260710.3403 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3403 2461231.8403 12.62 23:46:55.74 +26:57:52.8
105.61364 -33.72839 galactic Peg Second-epoch detections are separated by 1.0" and 6.9 pix
The object was found in VSX 3" Gaia DR3 2865005767849044352
Type: ROT
# Max. Min./Amp. JD0 Period
12.860 G 12.900 G M
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:46:55.74 +26:57:52.8: 13.56 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 23:46:55.74 +26:57:52.8: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2865005767849044352,2461231.8403,12.62,0.05,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 2865005767849044352 20260710.3403 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62421953 09.01.2026 02:58:42.567 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
First image: 2461049.62421953 09.01.2026 02:58:42.567 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Last image: 2461231.84053505 10.07.2026 08:10:12.228 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
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: 12 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): 11047
Objects passed selection criteria: 11000
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 7737.5
Average stars matched: 7552 (97.6026 %)
Memory usage VmPeak: 116684 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:30:44 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: 2461049.62421953 09.01.2026 02:58:42.567 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
First image: 2461049.62421953 09.01.2026 02:58:42.567 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Last image: 2461231.84053505 10.07.2026 08:10:12.228 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 68 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): 67810
Objects passed selection criteria: 67644
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 49455
Average stars matched: 47957 (96.971 %)
Memory usage VmPeak: 167448 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:35:04 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/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
SExtractor catalog cache: saved Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat to cache
SExtractor catalog cache: saved Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.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/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.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: 2461231.83999328
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_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits exists and is non-empty
Saving wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits to local_wcs_cache/
'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits exists and is non-empty
Saving wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits to local_wcs_cache/
'wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits' -> 'local_wcs_cache/wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits'
wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits exists and is non-empty
Saving wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits to local_wcs_cache/
'wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits' -> 'local_wcs_cache/wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits'
wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits exists and is non-empty
Saving wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits to local_wcs_cache/
'wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits' -> 'local_wcs_cache/wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits (1st reference image)
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.922 +29:59:56.50 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits (1st new image)
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:04.429 +29:59:47.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:59.922 +29:59:56.50
Second-epoch image center 00:00:04.429 +29:59:47.95
Angular distance between the image centers 0.0164 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits (2nd new image)
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:07.439 +29:59:44.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:59.922 +29:59:56.50
Second-epoch image center 00:00:07.439 +29:59:44.93
Angular distance between the image centers 0.0273 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 00:00:04.429 +29:59:47.95
Second-epoch second image center 00:00:07.439 +29:59:44.93
Angular distance between the image centers 0.01089 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.eXLP5o4FBO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits &> /tmp/tmp.pjkoNhVouJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits &> /tmp/tmp.jnrsUzsHvc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits &> /tmp/tmp.Xx8fYijYFR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.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_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits and wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits and wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
Found non-empty wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits and wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
The reference image (wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits) and catalog (wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat) found
'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat' -> 'wcsmag.cat'
Read 11750 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0033 to 359.9985 deg, Dec +24.3885 to +35.3076 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 0.0033 to 359.9985 deg, Dec 24.3885 to 35.3076 deg
Loaded 203938 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): 6500 out of 6882 total matches.
Matched with Tycho-2 6882 out of 11750 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.886800
a=0.000000 b=1.000000 c=22.886800
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11750 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0033 to 359.9985 deg, Dec +24.3885 to +35.3076 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 0.0033 to 359.9985 deg, Dec 24.3885 to 35.3076 deg
Loaded 203938 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): 6500 out of 6882 total matches.
Matched with Tycho-2 6882 out of 11750 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits:
Forced-photometry filter: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits -> calib.txt_param_ref_wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits (aperture=5.9)
Read 11742 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0032 to 359.9987 deg, Dec +24.3231 to +35.3219 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 0.0032 to 359.9987 deg, Dec 24.3231 to 35.3219 deg
Loaded 205335 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): 6495 out of 6888 total matches.
Matched with Tycho-2 6888 out of 11742 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits:
Forced-photometry filter: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits -> calib.txt_param_ref_wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
2.0 pix Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
2.6 pix fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
2.6 pix fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
2.0 pix wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
2.0 pix wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
Limiting magnitude estimates:
15.3 mag. Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
15.3 mag. Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
13.2 mag. fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
13.1 mag. fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.eXLP5o4FBO (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_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=866, bad_region=0, passed=11750
Got 11750 stars (including 10862 good ones) from the SExtractor catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 11750 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
RA wraps around 0/360 boundary: field RA 350.6514 through 0 to 9.6540, gap 9.6540 to 350.6514
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.6509 through 0 to 9.6544, gap 9.6544 to 350.6509
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits N_match=967 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.315 sigma_q3_arcsec=0.318 sigma_q4_arcsec=0.287 n_q1=226 n_q2=268 n_q3=232 n_q4=241 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pjkoNhVouJ (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_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits' -> 'wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits
WCS catalog name: wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=874, bad_region=0, passed=11742
Got 11742 stars (including 10850 good ones) from the SExtractor catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat
util/solve_plate_with_UCAC5 got 11742 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
RA wraps around 0/360 boundary: field RA 350.6337 through 0 to 9.6957, gap 9.6957 to 350.6337
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11523 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.6333 through 0 to 9.6962, gap 9.6962 to 350.6333
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits N_match=967 sigma_overall_arcsec=0.331 sigma_q1_arcsec=0.425 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.263 n_q1=223 n_q2=266 n_q3=233 n_q4=245 worst_quadrant_to_overall_ratio=1.284
The image catalog is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits -region wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jnrsUzsHvc (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_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.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_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
WCS catalog name: wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=171, bad_region=0, passed=3875
Got 3875 stars (including 3701 good ones) from the SExtractor catalog wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat
util/solve_plate_with_UCAC5 got 3875 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
RA wraps around 0/360 boundary: field RA 350.8407 through 0 to 9.8181, gap 9.8181 to 350.8407
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.8409 through 0 to 9.8185, gap 9.8185 to 350.8409
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits N_match=962 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.286 sigma_q4_arcsec=0.297 n_q1=287 n_q2=163 n_q3=272 n_q4=240 worst_quadrant_to_overall_ratio=1.355
The image catalog is written to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits -region wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Xx8fYijYFR (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_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.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_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
WCS catalog name: wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=153, bad_region=0, passed=3771
Got 3771 stars (including 3615 good ones) from the SExtractor catalog wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat
util/solve_plate_with_UCAC5 got 3771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.8501 through 0 to 9.8181, gap 9.8181 to 350.8501
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.8495 through 0 to 9.8185, gap 9.8185 to 350.8495
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits N_match=961 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.330 n_q1=276 n_q2=185 n_q3=277 n_q4=223 worst_quadrant_to_overall_ratio=1.410
The image catalog is written to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits -region wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat.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=Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits sigma_overall=0.334 worst_q_ratio=1.180
ref2=Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits sigma_overall=0.331 worst_q_ratio=1.284
new1=fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits sigma_overall=0.333 worst_q_ratio=1.355
new2=fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits sigma_overall=0.320 worst_q_ratio=1.410
reference average sigma_overall=0.3325 worst_q_ratio=1.232
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071_astrometric_residuals.png (967 matched stars from wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072_astrometric_residuals.png (967 matched stars from wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310_astrometric_residuals.png (962 matched stars from wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311_astrometric_residuals.png (961 matched stars from wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-09-25_20.00sec_0.00C_LIGHTs_0310.fits'
Saving fully-calibrated image wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-01-Q1b1x1_032157_TTUQ1b1x1_238292_Ms5ckExT/wcs_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311.fits'
Preparing the HTML report for the field Peg-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:04:40.22 +34:16:20.0: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-59-41_20.00sec_-14.90C_LIGHT_0072.fits at 00:04:40.22 +34:16:20.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 00:04:40.22 +34:16:20.0: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20681_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 20681_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 20687_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 20687_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 88788_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 88788_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 23:24:57.45 +30:53:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88789_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 88789_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 88922_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 88922_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 88984_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 88984_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 89012_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 89012_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 89058_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 89058_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 23:27:33.57 +29:12:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89129_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 89129_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 89163_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 89163_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 89178_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 89178_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 23:59:45.69 +30:37:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.772 2873331132455480832 359.94036803582 +30.62567451956 13.8861 13.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28160_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 28160_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 59776_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 59776_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 23664_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 23664_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 54017_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 54017_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 22060_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 22060_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 32662_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 32662_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 12663_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 12663_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 62987_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 62987_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25151_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25151_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25344_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25344_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53676_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 53676_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24120_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 24120_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 45822_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 45822_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28658_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 28658_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25862_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25862_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 24217_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 24217_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25957_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25957_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62517_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 62517_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 23720_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 23720_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 64298_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 64298_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 44176_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 44176_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55635_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 55635_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 59895_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 59895_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 64768_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 64768_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 59937_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 59937_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 27874_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 27874_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 64860_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 64860_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 66702_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 66702_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 61219_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 61219_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 44285_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 44285_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 57588_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 57588_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60921_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 60921_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65823_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 65823_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 68759_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 68759_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25718_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25718_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61188_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 61188_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 15550_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 15550_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62981_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 62981_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62788_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 62788_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30352_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 30352_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18248_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 18248_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63918_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 63918_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 60541_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 60541_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20905_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 20905_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25473_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25473_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 56465_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 56465_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25531_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25531_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25295_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25295_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 05482_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 05482_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 11112_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 11112_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 63549_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 63549_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 66857_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 66857_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 57827_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 57827_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 45109_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 45109_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 25194_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 25194_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 58451_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 58451_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 62470_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 62470_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 24314_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 24314_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 64303_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 64303_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 66904_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 66904_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 60007_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 60007_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 67112_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 67112_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 41779_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 41779_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 23:51:44.09 +29:45:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64585_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 64585_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 63009_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 63009_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 63810_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 63810_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 28967_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 28967_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 13774_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 13774_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 23:57:28.62 +33:32:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16176_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 16176_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 27506_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 27506_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 83475_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 83475_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 23:36:45.88 +27:37:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67378_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 67378_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 60338_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 60338_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 56831_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 56831_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 58713_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 58713_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 45311_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 45311_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 61863_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 61863_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 19372_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 19372_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 34605_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 34605_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
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Considering the candidate 64083_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 64083_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61964_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 61964_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45119_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 45119_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23237_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 23237_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23760_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 23760_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43795_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 43795_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30971_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 30971_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44135_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 44135_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22757_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 22757_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05436_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
The candidate 05436_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60671_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
Preparing report for the candidate 60671_fd_Peg-01-Q1b1x1_2026-07-10_03-10-12_20.00sec_0.00C_LIGHTs_0311
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 178s
Prepared the HTML report for the field Peg-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:13:55.62 +34:27:47.7
00:03:21.66 +33:50:35.9
23:58:27.90 +33:39:51.6
00:17:58.10 +33:06:48.7
00:17:49.65 +33:02:03.5
00:18:40.56 +32:46:11.7
00:05:18.44 +32:46:56.2
00:18:56.27 +32:25:42.5
00:20:07.89 +32:15:37.5
00:14:37.47 +32:15:21.9
00:19:50.15 +32:06:59.5
00:22:13.77 +32:01:34.7
00:19:14.36 +32:03:51.1
00:19:00.70 +32:04:08.7
00:18:22.88 +32:01:36.7
00:18:37.99 +32:00:41.1
00:19:14.58 +31:59:26.0
00:06:14.69 +32:02:23.4
00:03:33.93 +32:03:16.4
00:22:47.21 +31:48:29.2
00:18:23.07 +31:52:23.4
00:19:01.13 +31:51:06.7
00:06:04.71 +31:59:37.2
00:18:56.27 +31:48:54.1
00:18:36.04 +31:48:09.3
00:17:27.85 +31:48:25.1
00:19:51.38 +31:33:56.6
00:17:07.99 +31:33:49.7
00:19:57.42 +31:28:54.4
00:18:52.81 +31:26:00.4
00:16:42.66 +31:25:02.5
00:21:04.14 +31:10:04.9
00:18:07.64 +31:07:18.4
00:19:22.68 +30:52:09.5
00:19:37.88 +30:36:32.9
00:19:23.20 +29:21:22.9
00:19:42.87 +29:18:24.5
00:19:24.16 +29:17:59.7
00:19:27.51 +29:17:12.2
00:20:20.53 +29:09:06.8
00:18:36.10 +29:10:50.3
00:18:40.31 +29:08:53.9
00:20:17.17 +29:02:52.8
23:48:29.54 +26:05:23.8
23:40:55.12 +26:08:06.5
23:46:26.30 +26:19:49.2
23:48:01.39 +26:27:20.0
23:45:36.36 +26:28:02.6
23:48:18.33 +26:34:42.3
23:39:46.00 +26:36:10.2
23:40:04.98 +26:41:09.5
23:46:11.31 +26:43:31.0
23:45:07.75 +26:50:58.3
23:39:33.17 +26:53:45.2
23:48:46.52 +26:53:07.3
23:39:27.28 +26:52:12.5
23:38:54.11 +26:55:49.7
23:46:55.74 +26:57:52.8
23:50:54.35 +26:59:36.3
23:47:11.10 +27:01:31.2
23:39:16.36 +27:01:48.4
23:43:48.31 +27:06:29.2
23:49:26.26 +27:08:30.7
23:37:59.61 +27:11:22.5
23:47:26.38 +27:13:25.2
23:49:10.92 +27:14:47.4
23:37:10.23 +27:28:14.2
23:38:20.07 +27:15:17.9
23:38:30.96 +27:18:04.2
23:45:14.18 +27:19:31.9
23:47:46.97 +27:23:36.1
23:53:02.20 +27:21:59.7
23:37:59.10 +27:25:35.2
23:37:39.46 +27:28:03.3
23:44:21.56 +27:26:31.3
23:44:15.99 +27:27:38.4
23:44:51.60 +27:30:37.7
23:45:11.33 +27:31:15.2
23:44:47.18 +27:37:17.5
23:38:59.82 +27:45:30.3
23:44:04.35 +27:45:46.2
23:39:08.12 +27:45:51.7
23:36:18.93 +27:47:00.4
23:36:47.87 +27:49:40.5
23:59:13.86 +28:35:05.4
########### Completed Peg-01-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 ####
00:19:57.42 +31:28:54.4
23:45:07.75 +26:50:58.3
00:22:13.77 +32:01:34.7
23:40:55.12 +26:08:06.5
00:20:07.89 +32:15:37.5
00:19:22.68 +30:52:09.5
23:58:27.90 +33:39:51.6
23:38:20.07 +27:15:17.9
00:06:14.69 +32:02:23.4
00:18:23.07 +31:52:23.4
23:48:29.54 +26:05:23.8
00:18:22.88 +32:01:36.7
00:20:17.17 +29:02:52.8
00:18:52.81 +31:26:00.4
00:18:36.04 +31:48:09.3
00:18:37.99 +32:00:41.1
00:17:27.85 +31:48:25.1
23:47:26.38 +27:13:25.2
00:19:14.36 +32:03:51.1
23:37:39.46 +27:28:03.3
00:19:24.16 +29:17:59.7
23:46:26.30 +26:19:49.2
23:39:33.17 +26:53:45.2
23:44:51.60 +27:30:37.7
23:48:46.52 +26:53:07.3
00:17:07.99 +31:33:49.7
23:45:11.33 +27:31:15.2
23:38:59.82 +27:45:30.3
23:39:16.36 +27:01:48.4
00:19:27.51 +29:17:12.2
23:48:18.33 +26:34:42.3
23:50:54.35 +26:59:36.3
23:44:47.18 +27:37:17.5
23:59:13.86 +28:35:05.4
00:18:56.27 +31:48:54.1
23:47:11.10 +27:01:31.2
00:17:58.10 +33:06:48.7
23:37:10.23 +27:28:14.2
23:49:10.92 +27:14:47.4
00:21:04.14 +31:10:04.9
00:18:40.56 +32:46:11.7
23:53:02.20 +27:21:59.7
23:38:54.11 +26:55:49.7
00:18:56.27 +32:25:42.5
00:19:01.13 +31:51:06.7
23:48:01.39 +26:27:20.0
00:06:04.71 +31:59:37.2
00:22:47.21 +31:48:29.2
00:13:55.62 +34:27:47.7
00:03:21.66 +33:50:35.9
23:45:14.18 +27:19:31.9
23:44:04.35 +27:45:46.2
23:39:46.00 +26:36:10.2
00:20:20.53 +29:09:06.8
00:03:33.93 +32:03:16.4
23:40:04.98 +26:41:09.5
23:37:59.61 +27:11:22.5
00:19:14.58 +31:59:26.0
23:44:21.56 +27:26:31.3
23:39:08.12 +27:45:51.7
23:39:27.28 +26:52:12.5
23:36:18.93 +27:47:00.4
23:44:15.99 +27:27:38.4
23:38:30.96 +27:18:04.2
23:47:46.97 +27:23:36.1
00:16:42.66 +31:25:02.5
00:17:49.65 +33:02:03.5
00:19:51.38 +31:33:56.6
23:36:47.87 +27:49:40.5
23:45:36.36 +26:28:02.6
23:46:11.31 +26:43:31.0
00:18:40.31 +29:08:53.9
23:43:48.31 +27:06:29.2
00:05:18.44 +32:46:56.2
00:19:37.88 +30:36:32.9
23:37:59.10 +27:25:35.2
23:49:26.26 +27:08:30.7
00:18:36.10 +29:10:50.3
00:19:50.15 +32:06:59.5
00:19:00.70 +32:04:08.7
00:19:23.20 +29:21:22.9
00:18:07.64 +31:07:18.4
00:19:42.87 +29:18:24.5
00:14:37.47 +32:15:21.9
23:46:55.74 +26:57:52.8
###################################################################################
00:19:57.42 +31:28:54.4 -- not an asteroid (will add it to exclusion list)
23:45:07.75 +26:50:58.3 -- not an asteroid (will add it to exclusion list)
00:22:13.77 +32:01:34.7 -- not an asteroid (will add it to exclusion list)
23:40:55.12 +26:08:06.5 -- not an asteroid (will add it to exclusion list)
00:20:07.89 +32:15:37.5 -- not an asteroid (will add it to exclusion list)
00:19:22.68 +30:52:09.5 -- not an asteroid (will add it to exclusion list)
23:58:27.90 +33:39:51.6 -- not an asteroid (will add it to exclusion list)
23:38:20.07 +27:15:17.9 -- not an asteroid (will add it to exclusion list)
00:06:14.69 +32:02:23.4 -- not an asteroid (will add it to exclusion list)
00:18:23.07 +31:52:23.4 -- not an asteroid (will add it to exclusion list)
23:48:29.54 +26:05:23.8 -- not an asteroid (will add it to exclusion list)
00:18:22.88 +32:01:36.7 -- not an asteroid (will add it to exclusion list)
00:20:17.17 +29:02:52.8 -- not an asteroid (will add it to exclusion list)
00:18:52.81 +31:26:00.4 -- not an asteroid (will add it to exclusion list)
00:18:36.04 +31:48:09.3 -- not an asteroid (will add it to exclusion list)
00:18:37.99 +32:00:41.1 -- not an asteroid (will add it to exclusion list)
00:17:27.85 +31:48:25.1 -- not an asteroid (will add it to exclusion list)
23:47:26.38 +27:13:25.2 -- not an asteroid (will add it to exclusion list)
00:19:14.36 +32:03:51.1 -- not an asteroid (will add it to exclusion list)
23:37:39.46 +27:28:03.3 -- not an asteroid (will add it to exclusion list)
00:19:24.16 +29:17:59.7 -- not an asteroid (will add it to exclusion list)
23:46:26.30 +26:19:49.2 -- not an asteroid (will add it to exclusion list)
23:39:33.17 +26:53:45.2 -- not an asteroid (will add it to exclusion list)
23:44:51.60 +27:30:37.7 -- not an asteroid (will add it to exclusion list)
23:48:46.52 +26:53:07.3 -- not an asteroid (will add it to exclusion list)
00:17:07.99 +31:33:49.7 -- not an asteroid (will add it to exclusion list)
23:45:11.33 +27:31:15.2 -- not an asteroid (will add it to exclusion list)
23:38:59.82 +27:45:30.3 -- not an asteroid (will add it to exclusion list)
23:39:16.36 +27:01:48.4 -- not an asteroid (will add it to exclusion list)
00:19:27.51 +29:17:12.2 -- not an asteroid (will add it to exclusion list)
23:48:18.33 +26:34:42.3 -- not an asteroid (will add it to exclusion list)
23:50:54.35 +26:59:36.3 -- not an asteroid (will add it to exclusion list)
23:44:47.18 +27:37:17.5 -- not an asteroid (will add it to exclusion list)
23:59:13.86 +28:35:05.4 -- not an asteroid (will add it to exclusion list)
00:18:56.27 +31:48:54.1 -- not an asteroid (will add it to exclusion list)
23:47:11.10 +27:01:31.2 -- not an asteroid (will add it to exclusion list)
00:17:58.10 +33:06:48.7 -- not an asteroid (will add it to exclusion list)
23:37:10.23 +27:28:14.2 -- not an asteroid (will add it to exclusion list)
23:49:10.92 +27:14:47.4 -- not an asteroid (will add it to exclusion list)
00:21:04.14 +31:10:04.9 -- not an asteroid (will add it to exclusion list)
00:18:40.56 +32:46:11.7 -- not an asteroid (will add it to exclusion list)
23:53:02.20 +27:21:59.7 -- not an asteroid (will add it to exclusion list)
23:38:54.11 +26:55:49.7 -- not an asteroid (will add it to exclusion list)
00:18:56.27 +32:25:42.5 -- not an asteroid (will add it to exclusion list)
00:19:01.13 +31:51:06.7 -- not an asteroid (will add it to exclusion list)
23:48:01.39 +26:27:20.0 -- not an asteroid (will add it to exclusion list)
00:06:04.71 +31:59:37.2 -- not an asteroid (will add it to exclusion list)
00:22:47.21 +31:48:29.2 -- not an asteroid (will add it to exclusion list)
00:13:55.62 +34:27:47.7 -- not an asteroid (will add it to exclusion list)
00:03:21.66 +33:50:35.9 -- not an asteroid (will add it to exclusion list)
23:45:14.18 +27:19:31.9 -- not an asteroid (will add it to exclusion list)
23:44:04.35 +27:45:46.2 -- not an asteroid (will add it to exclusion list)
23:39:46.00 +26:36:10.2 -- not an asteroid (will add it to exclusion list)
00:20:20.53 +29:09:06.8 -- not an asteroid (will add it to exclusion list)
00:03:33.93 +32:03:16.4 -- not an asteroid (will add it to exclusion list)
23:40:04.98 +26:41:09.5 -- not an asteroid (will add it to exclusion list)
23:37:59.61 +27:11:22.5 -- not an asteroid (will add it to exclusion list)
00:19:14.58 +31:59:26.0 -- not an asteroid (will add it to exclusion list)
23:44:21.56 +27:26:31.3 -- not an asteroid (will add it to exclusion list)
23:39:08.12 +27:45:51.7 -- not an asteroid (will add it to exclusion list)
23:39:27.28 +26:52:12.5 -- not an asteroid (will add it to exclusion list)
23:36:18.93 +27:47:00.4 -- not an asteroid (will add it to exclusion list)
23:44:15.99 +27:27:38.4 -- not an asteroid (will add it to exclusion list)
23:38:30.96 +27:18:04.2 -- not an asteroid (will add it to exclusion list)
23:47:46.97 +27:23:36.1 -- not an asteroid (will add it to exclusion list)
00:16:42.66 +31:25:02.5 -- not an asteroid (will add it to exclusion list)
00:17:49.65 +33:02:03.5 -- not an asteroid (will add it to exclusion list)
00:19:51.38 +31:33:56.6 -- not an asteroid (will add it to exclusion list)
23:36:47.87 +27:49:40.5 -- not an asteroid (will add it to exclusion list)
23:45:36.36 +26:28:02.6 -- not an asteroid (will add it to exclusion list)
23:46:11.31 +26:43:31.0 -- not an asteroid (will add it to exclusion list)
00:18:40.31 +29:08:53.9 -- not an asteroid (will add it to exclusion list)
23:43:48.31 +27:06:29.2 -- not an asteroid (will add it to exclusion list)
00:05:18.44 +32:46:56.2 -- not an asteroid (will add it to exclusion list)
00:19:37.88 +30:36:32.9 -- not an asteroid (will add it to exclusion list)
23:37:59.10 +27:25:35.2 -- not an asteroid (will add it to exclusion list)
23:49:26.26 +27:08:30.7 -- not an asteroid (will add it to exclusion list)
00:18:36.10 +29:10:50.3 -- not an asteroid (will add it to exclusion list)
00:19:50.15 +32:06:59.5 -- not an asteroid (will add it to exclusion list)
00:19:00.70 +32:04:08.7 -- not an asteroid (will add it to exclusion list)
00:19:23.20 +29:21:22.9 -- not an asteroid (will add it to exclusion list)
00:18:07.64 +31:07:18.4 -- not an asteroid (will add it to exclusion list)
00:19:42.87 +29:18:24.5 -- not an asteroid (will add it to exclusion list)
00:14:37.47 +32:15:21.9 -- not an asteroid (will add it to exclusion list)
23:46:55.74 +26:57:52.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:03:21.66 +33:50:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:33.93 +32:03:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:18.44 +32:46:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:04.71 +31:59:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:14.69 +32:02:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:55.62 +34:27:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:37.47 +32:15:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:42.66 +31:25:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:07.99 +31:33:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:27.85 +31:48:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:49.65 +33:02:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:58.10 +33:06:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:07.64 +31:07:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:22.88 +32:01:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:23.07 +31:52:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:36.04 +31:48:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:36.10 +29:10:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:37.99 +32:00:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:40.31 +29:08:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:40.56 +32:46:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:52.81 +31:26:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:56.27 +31:48:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:56.27 +32:25:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:00.70 +32:04:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:01.13 +31:51:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:14.36 +32:03:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:14.58 +31:59:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:22.68 +30:52:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:23.20 +29:21:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:24.16 +29:17:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:27.51 +29:17:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:37.88 +30:36:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:42.87 +29:18:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:50.15 +32:06:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:51.38 +31:33:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:57.42 +31:28:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:07.89 +32:15:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:17.17 +29:02:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:20.53 +29:09:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:04.14 +31:10:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:13.77 +32:01:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:47.21 +31:48:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:18.93 +27:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:47.87 +27:49:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:10.23 +27:28:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:39.46 +27:28:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:59.10 +27:25:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:59.61 +27:11:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:20.07 +27:15:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:30.96 +27:18:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:54.11 +26:55:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:59.82 +27:45:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:08.12 +27:45:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:16.36 +27:01:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:27.28 +26:52:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:33.17 +26:53:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:46.00 +26:36:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:04.98 +26:41:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:55.12 +26:08:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:48.31 +27:06:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:04.35 +27:45:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:15.99 +27:27:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:21.56 +27:26:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:47.18 +27:37:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:51.60 +27:30:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:07.75 +26:50:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:11.33 +27:31:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:14.18 +27:19:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:36.36 +26:28:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:11.31 +26:43:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:26.30 +26:19:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:55.74 +26:57:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:11.10 +27:01:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:26.38 +27:13:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:46.97 +27:23:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:01.39 +26:27:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:18.33 +26:34:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:29.54 +26:05:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:46.52 +26:53:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:10.92 +27:14:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:26.26 +27:08:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:54.35 +26:59:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:02.20 +27:21:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:27.90 +33:39:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:13.86 +28:35:05.4 -- 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)
00:03:21.66 +33:50:35.9 -- not a known variable star
00:03:33.93 +32:03:16.4 -- not a known variable star
00:05:18.44 +32:46:56.2 -- not a known variable star
00:06:04.71 +31:59:37.2 -- not a known variable star
00:06:14.69 +32:02:23.4 -- not a known variable star
00:13:55.62 +34:27:47.7 -- not a known variable star
00:14:37.47 +32:15:21.9 -- not a known variable star
00:16:42.66 +31:25:02.5 -- not a known variable star
00:17:07.99 +31:33:49.7 -- not a known variable star
00:17:27.85 +31:48:25.1 -- a known variable star
00:17:49.65 +33:02:03.5 -- not a known variable star
00:17:58.10 +33:06:48.7 -- a known variable star
00:18:07.64 +31:07:18.4 -- not a known variable star
00:18:22.88 +32:01:36.7 -- not a known variable star
00:18:23.07 +31:52:23.4 -- not a known variable star
00:18:36.04 +31:48:09.3 -- not a known variable star
00:18:36.10 +29:10:50.3 -- not a known variable star
00:18:37.99 +32:00:41.1 -- a known variable star
00:18:40.31 +29:08:53.9 -- not a known variable star
00:18:40.56 +32:46:11.7 -- not a known variable star
00:18:52.81 +31:26:00.4 -- not a known variable star
00:18:56.27 +31:48:54.1 -- not a known variable star
00:18:56.27 +32:25:42.5 -- not a known variable star
00:19:00.70 +32:04:08.7 -- not a known variable star
00:19:01.13 +31:51:06.7 -- not a known variable star
00:19:14.36 +32:03:51.1 -- not a known variable star
00:19:14.58 +31:59:26.0 -- not a known variable star
00:19:22.68 +30:52:09.5 -- not a known variable star
00:19:23.20 +29:21:22.9 -- not a known variable star
00:19:24.16 +29:17:59.7 -- not a known variable star
00:19:27.51 +29:17:12.2 -- not a known variable star
00:19:37.88 +30:36:32.9 -- not a known variable star
00:19:42.87 +29:18:24.5 -- a known variable star
00:19:50.15 +32:06:59.5 -- not a known variable star
00:19:51.38 +31:33:56.6 -- not a known variable star
00:19:57.42 +31:28:54.4 -- not a known variable star
00:20:07.89 +32:15:37.5 -- a known variable star
00:20:17.17 +29:02:52.8 -- not a known variable star
00:20:20.53 +29:09:06.8 -- not a known variable star
00:21:04.14 +31:10:04.9 -- not a known variable star
00:22:13.77 +32:01:34.7 -- not a known variable star
00:22:47.21 +31:48:29.2 -- not a known variable star
23:36:18.93 +27:47:00.4 -- not a known variable star
23:36:47.87 +27:49:40.5 -- not a known variable star
23:37:10.23 +27:28:14.2 -- not a known variable star
23:37:39.46 +27:28:03.3 -- not a known variable star
23:37:59.10 +27:25:35.2 -- not a known variable star
23:37:59.61 +27:11:22.5 -- not a known variable star
23:38:20.07 +27:15:17.9 -- not a known variable star
23:38:30.96 +27:18:04.2 -- not a known variable star
23:38:54.11 +26:55:49.7 -- not a known variable star
23:38:59.82 +27:45:30.3 -- not a known variable star
23:39:08.12 +27:45:51.7 -- not a known variable star
23:39:16.36 +27:01:48.4 -- not a known variable star
23:39:27.28 +26:52:12.5 -- not a known variable star
23:39:33.17 +26:53:45.2 -- not a known variable star
23:39:46.00 +26:36:10.2 -- not a known variable star
23:40:04.98 +26:41:09.5 -- not a known variable star
23:40:55.12 +26:08:06.5 -- not a known variable star
23:43:48.31 +27:06:29.2 -- a known variable star
23:44:04.35 +27:45:46.2 -- not a known variable star
23:44:15.99 +27:27:38.4 -- not a known variable star
23:44:21.56 +27:26:31.3 -- not a known variable star
23:44:47.18 +27:37:17.5 -- not a known variable star
23:44:51.60 +27:30:37.7 -- not a known variable star
23:45:07.75 +26:50:58.3 -- not a known variable star
23:45:11.33 +27:31:15.2 -- not a known variable star
23:45:14.18 +27:19:31.9 -- not a known variable star
23:45:36.36 +26:28:02.6 -- not a known variable star
23:46:11.31 +26:43:31.0 -- not a known variable star
23:46:26.30 +26:19:49.2 -- not a known variable star
23:46:55.74 +26:57:52.8 -- a known variable star
23:47:11.10 +27:01:31.2 -- not a known variable star
23:47:26.38 +27:13:25.2 -- not a known variable star
23:47:46.97 +27:23:36.1 -- not a known variable star
23:48:01.39 +26:27:20.0 -- not a known variable star
23:48:18.33 +26:34:42.3 -- not a known variable star
23:48:29.54 +26:05:23.8 -- not a known variable star
23:48:46.52 +26:53:07.3 -- not a known variable star
23:49:10.92 +27:14:47.4 -- not a known variable star
23:49:26.26 +27:08:30.7 -- not a known variable star
23:50:54.35 +26:59:36.3 -- not a known variable star
23:53:02.20 +27:21:59.7 -- not a known variable star
23:58:27.90 +33:39:51.6 -- not a known variable star
23:59:13.86 +28:35:05.4 -- not a known variable star
Found 78 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
85 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 85 (excluding asteroids and hot pixels, 78 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)2461231.83999328 -observatory V36
07:32:18.37 +17:08:02.8 Mercury (5.1mag)
10:11:36.07 +12:41:16.5 Venus (-4.1mag)
04:24:08.43 +21:25:07.4 Mars (1.3mag)
08:16:39.98 +20:11:30.8 Jupiter (-1.8mag)
00:55:50.84 +03:20:28.6 Saturn (0.7mag)
04:07:13.91 +20:45:03.0 Uranus (5.8mag)
00:17:01.50 +00:20:41.2 Neptune (7.8mag)
20:30:55.00 -23:18:00.3 Pluto (14.4mag)
03:11:04.74 +22:17:01.2 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 03:30 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461231.83999328:
08:16:46.57 +20:11:08.0 Io (6.1mag)
08:16:42.65 +20:11:22.7 Europa (6.3mag)
08:16:57.03 +20:10:29.2 Ganymede (5.6mag)
08:17:08.00 +20:09:47.3 Callisto (6.8mag)
08:15:11.50 +19:55:40.2 Himalia (15.7mag)
08:16:38.98 +20:11:35.5 Thebe (16.6mag)
08:14:32.84 +20:00:09.8 Elara (17.6mag)
08:20:12.18 +20:05:41.3 Pasiphae (17.8mag)
08:21:37.87 +20:16:35.7 Carme (19.0mag)
00:55:40.68 +03:20:19.5 Titan (8.5mag)
00:55:45.60 +03:20:31.8 Rhea (9.8mag)
00:55:20.15 +03:19:37.6 Iapetus (11.2mag)
00:56:00.11 +03:20:47.6 Hyperion (14.5mag)
00:55:51.58 +03:17:42.5 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 03:30 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.83999328:
17:46:08.96 -32:59:39.6 JWST
16:13:18.92 +48:56:44.3 Chandra
02:37:08.95 +62:31:14.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 03:30 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.83999328 -observatory V36
02:36:15.18 +14:25:36.8 17.9mag P/1996 R2 (Lagerkvist)
18:17:56.92 -34:21:44.3 13.7mag P/2010 H2 (Vales)
06:25:39.78 -68:08:22.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:48.13 +32:26:48.3 17.6mag C/2017 K2 (PANSTARRS)
17:03:07.16 +16:02:54.7 18.0mag C/2021 G2 (ATLAS)
01:47:44.36 +08:11:51.1 15.4mag P/2021 N1 (ZTF)
22:59:32.30 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:23.17 +26:55:35.0 16.7mag C/2022 N2 (PANSTARRS)
09:55:30.30 +29:46:53.1 16.8mag C/2022 QE78 (ATLAS)
09:09:43.66 +04:59:56.4 17.8mag C/2022 R6 (PANSTARRS)
18:07:13.51 +21:17:39.5 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.30 -11:23:15.1 17.7mag P/2023 B1 (PANSTARRS)
21:49:14.93 +67:37:16.9 17.8mag C/2023 H5 (Lemmon)
16:30:54.53 -10:04:37.2 13.9mag C/2023 R1 (PANSTARRS)
08:00:37.80 +65:42:28.1 17.9mag C/2024 A1 (ATLAS)
07:32:47.94 +30:00:09.8 14.6mag C/2024 E1 (Wierzchos)
15:16:19.91 +15:19:40.9 17.5mag C/2024 G6 (ATLAS)
19:41:19.48 +39:23:26.7 13.8mag C/2024 J3 (ATLAS)
21:47:35.69 +46:00:05.3 17.8mag C/2024 R4 (PANSTARRS)
04:49:37.68 -13:47:47.2 15.7mag C/2024 T5 (ATLAS)
06:34:33.79 +29:04:18.6 18.0mag C/2025 J1 (Borisov)
07:14:19.84 -12:53:19.0 16.5mag C/2025 R3 (PANSTARRS)
09:56:04.68 +22:26:14.5 17.6mag C/2025 V2 (Rankin)
12:44:36.78 +03:56:17.9 17.1mag C/2025 Y1 (ATLAS)
16:51:59.25 +79:07:12.3 17.4mag C/2026 A2 (Bok)
02:46:15.78 +45:14:21.5 16.7mag C/2026 B2 (Sun-Gao)
11:25:30.21 +04:32:31.2 16.9mag A/2026 E1
21:19:01.13 -15:04:19.9 7.3mag 10P/Tempel
11:13:26.96 -01:53:12.1 16.1mag 29P/Schwassmann-Wachmann
04:00:09.28 +29:33:06.6 17.8mag 47P/Ashbrook-Jackson
10:08:03.06 +14:00:55.1 17.0mag 63P/Wild
00:48:21.43 -05:05:35.8 15.5mag 65P/Gunn
08:26:54.89 +34:13:09.8 17.9mag 76P/West-Kohoutek-Ikemura
04:27:22.11 +20:10:41.2 13.7mag 78P/Gehrels
02:22:18.86 +10:36:28.1 16.2mag 88P/Howell
06:35:29.63 +30:32:07.7 15.7mag 93P/Lovas
04:20:57.57 +31:07:20.8 16.9mag 114P/Wiseman-Skiff
08:08:39.86 +30:42:17.5 15.3mag 123P/West-Hartley
10:48:06.50 +01:11:30.9 16.8mag 124P/Mrkos
04:51:42.50 +20:48:45.4 16.2mag 128P/Shoemaker-Holt
05:36:13.94 +19:42:50.9 17.8mag 131P/Mueller
00:01:32.52 +02:56:05.1 17.9mag 139P/Vaisala-Oterma
07:13:30.97 +17:01:24.1 15.5mag 141P-D/Machholz
03:16:50.62 -21:06:25.0 15.5mag 161P/Hartley-IRAS
05:33:01.14 +33:56:45.3 15.3mag 162P/SidingSpring
19:04:30.27 +15:04:30.4 14.7mag 169P/NEAT
01:41:00.05 +07:35:50.1 17.7mag 220P/McNaught
16:35:58.24 -08:23:05.7 17.0mag 235P/LINEAR
08:45:15.57 +33:18:02.1 17.9mag 240P/NEAT
20:42:10.84 -49:34:04.4 17.8mag 259P/Garradd
01:59:16.32 +12:05:20.4 15.7mag 260P/McNaught
05:37:11.32 +36:50:30.8 17.4mag 295P/LINEAR
15:06:36.83 +06:03:28.8 17.6mag 391P/Kowalski
08:34:35.55 +19:40:38.2 17.9mag 450P/LONEOS
07:51:44.82 +39:13:01.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 03:30 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
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
-rw-r--r-- 1 apache apache 5.6K Jul 10 03:30 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 03:30 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:36:21.258 +13:42:31.91 AT 2026sqg 2026-07-06.96 17.376
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
-rw-r--r-- 1 apache apache 30K Jul 10 03:30 tns_transients_list.txt
