This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT
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 10.3916 2461231.8916 11.68 22:29:33.33 -11:22:31.9
51.26669 -53.17951 galactic Aqr Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate -0 -0 0 11.9 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:33.33 -11:22:31.9: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:33.33 -11:22:31.9: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461231.8916,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3916 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.02 22:26:36.54 -08:06:48.5
55.13075 -50.83093 galactic Aqr Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:26:36.54 -08:06:48.5 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.038 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:26:36.54 -08:06:48.5: 13.03 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:26:36.54 -08:06:48.5: 12.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.92 +/- 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,2461231.8916,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.70 21:55:22.75 -13:01:45.4
42.88853 -46.58280 galactic Cap Second-epoch detections are separated by 1.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:22.75 -13:01:45.4 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.030 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:55:22.75 -13:01:45.4: 12.89 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:55:22.75 -13:01:45.4: 13.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 10.3916* 21 55 22.75 -13 01 45.4 11.7 U Cap 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,2461231.8916,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.52 22:25:54.36 -08:03:04.4
55.06031 -50.65158 galactic Aqr Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:25:54.36 -08:03:04.4 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:25:54.36 -08:03:04.4: 13.77 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:25:54.36 -08:03:04.4: 13.67 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.69 22:31:07.94 -08:34:00.8
55.52238 -52.01323 galactic Aqr Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2621310732222285696 | 22:31:07.92 -08:34:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.271+/-0.029 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:31:07.94 -08:34:00.8: 12.66 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:31:07.94 -08:34:00.8: 12.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2621310732222285696,2461231.8916,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2621310732222285696 20260710.3916 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 10.96 21:51:33.47 -12:49:17.4
42.57217 -45.65432 galactic Cap Second-epoch detections are separated by 1.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843822509758898816 | 21:51:33.46 -12:49:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.030 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:51:33.47 -12:49:17.4: 11.89 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:51:33.47 -12:49:17.4: 12.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 51 33.47 -12 49 17.4 11.0 U Cap 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 6843822509758898816,2461231.8916,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843822509758898816 20260710.3916 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.41 21:53:24.58 -13:13:09.4
42.33837 -46.23332 galactic Cap Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840792015194731008 | 21:53:24.59 -13:13:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.382+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:24.58 -13:13:09.4: 12.43 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:24.58 -13:13:09.4: 12.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 24.58 -13 13 09.4 11.4 U Cap 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 6840792015194731008,2461231.8916,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840792015194731008 20260710.3916 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.12 22:26:42.91 -08:34:16.1
54.54722 -51.10498 galactic Aqr Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:26:42.91 -08:34:16.1 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:26:42.91 -08:34:16.1: 13.10 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:26:42.91 -08:34:16.1: 13.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.09 +/- 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,2461231.8916,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 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 10.3916 2461231.8916 11.53 21:57:48.08 -13:37:59.8
42.46434 -47.37542 galactic Cap Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840473912737560320 | 21:57:48.11 -13:37:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.031 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:57:48.08 -13:37:59.8: 12.43 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:57:48.08 -13:37:59.8: 12.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 57 48.08 -13 37 59.8 11.5 U Cap 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 6840473912737560320,2461231.8916,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840473912737560320 20260710.3916 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.46 21:56:19.64 -13:01:44.6
43.03588 -46.79045 galactic Cap Second-epoch detections are separated by 0.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840834518190937472 | 21:56:19.63 -13:01:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.646+/-0.028 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:19.64 -13:01:44.6: 12.43 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:56:19.64 -13:01:44.6: 12.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 56 19.64 -13 01 44.6 11.5 U Cap 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 6840834518190937472,2461231.8916,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840834518190937472 20260710.3916 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.71 21:53:15.99 -13:35:35.3
41.82798 -46.36229 galactic Cap Second-epoch detections are separated by 1.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:15.99 -13:35:35.3 (user input) | T | P | (position from user input) J-Ks=0.315+/-0.034 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:15.99 -13:35:35.3: 12.98 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:15.99 -13:35:35.3: 13.12 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 15.99 -13 35 35.3 11.7 U Cap 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,2461231.8916,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.20 21:49:51.83 -12:53:19.3
42.22970 -45.31177 galactic Cap Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.4607-12.8975 | 21:49:51.88 -12:53:18.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.006+/-0.033 (A)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:51.83 -12:53:19.3: 12.20 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:51.83 -12:53:19.3: 12.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.23 +/- 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 10.3916* 21 49 51.83 -12 53 19.3 11.2 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.4607-12.8975,2461231.8916,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4607-12.8975 20260710.3916 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.04 22:27:16.71 -08:18:07.5
55.02695 -51.07329 galactic Aqr Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:16.71 -08:18:07.5 (user input) | T | P | (position from user input) J-Ks=0.607+/-0.035 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:16.71 -08:18:07.5: 12.98 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:16.71 -08:18:07.5: 12.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 10.62 21:53:18.83 -13:12:29.0
42.33844 -46.20744 galactic Cap Second-epoch detections are separated by 0.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840792255712899328 | 21:53:18.81 -13:12:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:18.83 -13:12:29.0: 11.55 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:18.83 -13:12:29.0: 11.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 18.83 -13 12 29.0 10.6 U Cap 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 6840792255712899328,2461231.8916,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840792255712899328 20260710.3916 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.85 22:30:17.73 -08:29:52.2
55.42895 -51.80287 galactic Aqr Second-epoch detections are separated by 0.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:30:17.73 -08:29:52.2 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.031 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:30:17.73 -08:29:52.2: 12.86 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:30:17.73 -08:29:52.2: 12.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.20 21:50:16.80 -13:24:51.9
41.61510 -45.62940 galactic Cap Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840401001372305920 | 21:50:16.78 -13:24:51.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.033 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:16.80 -13:24:51.9: 12.17 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:50:16.80 -13:24:51.9: 12.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 50 16.80 -13 24 51.9 11.2 U Cap 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 6840401001372305920,2461231.8916,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840401001372305920 20260710.3916 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.88 22:27:26.84 -08:39:16.6
54.59394 -51.30212 galactic Aqr Second-epoch detections are separated by 0.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:26.84 -08:39:16.6 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.031 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:26.84 -08:39:16.6: 12.82 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:26.84 -08:39:16.6: 12.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.21 22:29:50.57 -08:53:49.1
54.79001 -51.92999 galactic Aqr Second-epoch detections are separated by 0.3" and 3.5 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 | Large-amplitude variable Gaia DR2 2621202086729527936 | 22:29:50.57 -08:53:49.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.526+/-0.035 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:50.57 -08:53:49.1: 13.07 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:50.57 -08:53:49.1: 13.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.04 +/- 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
Large-amplitude variable Gaia DR2 2621202086729527936,2461231.8916,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2621202086729527936 20260710.3916 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.69 21:54:47.77 -13:11:56.2
42.57658 -46.52877 galactic Cap Second-epoch detections are separated by 2.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:47.77 -13:11:56.2 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:47.77 -13:11:56.2: 12.60 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:54:47.77 -13:11:56.2: 12.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 54 47.77 -13 11 56.2 11.7 U Cap 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,2461231.8916,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.31 22:27:54.04 -08:41:42.4
54.63798 -51.41804 galactic Aqr Second-epoch detections are separated by 2.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:54.04 -08:41:42.4 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:54.04 -08:41:42.4: 13.39 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:54.04 -08:41:42.4: 13.28 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.34 +/- 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,2461231.8916,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.52 21:51:15.10 -12:55:38.4
42.38942 -45.63321 galactic Cap Second-epoch detections are separated by 1.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843796572452116992 | 21:51:15.15 -12:55:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.030 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:51:15.10 -12:55:38.4: 12.42 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:51:15.10 -12:55:38.4: 12.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 51 15.10 -12 55 38.4 11.5 U Cap 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 6843796572452116992,2461231.8916,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843796572452116992 20260710.3916 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.37 21:50:06.34 -12:42:20.0
42.50058 -45.28514 galactic Cap Second-epoch detections are separated by 0.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843862710652787072 | 21:50:06.34 -12:42:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.678+/-0.034 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:06.34 -12:42:20.0: 12.41 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:50:06.34 -12:42:20.0: 12.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.47 +/- 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!
TCP 2026 07 10.3916* 21 50 06.34 -12 42 20.0 11.4 U Cap 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 6843862710652787072,2461231.8916,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843862710652787072 20260710.3916 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.19 22:28:11.01 -09:06:56.3
54.13206 -51.70580 galactic Aqr Second-epoch detections are separated by 0.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:28:11.01 -09:06:56.3 (user input) | T | P | (position from user input) J-Ks=0.670+/-0.033 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:28:11.01 -09:06:56.3: 13.24 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:28:11.01 -09:06:56.3: 13.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.06 22:25:54.60 -08:05:12.2
55.01453 -50.67206 galactic Aqr Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J336.4734-08.0863 | 22:25:54.60 -08:05:12.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.464+/-0.030 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:25:54.60 -08:05:12.2: 12.94 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:25:54.60 -08:05:12.2: 13.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J336.4734-08.0863,2461231.8916,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J336.4734-08.0863 20260710.3916 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.15 22:27:57.51 -09:01:07.5
54.21467 -51.60657 galactic Aqr Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:57.51 -09:01:07.5 (user input) | T | P | (position from user input) J-Ks=0.288+/-0.034 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:57.51 -09:01:07.5: 13.25 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:57.51 -09:01:07.5: 13.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 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 10.3916 2461231.8916 12.30 22:25:48.34 -08:32:51.0
54.38326 -50.90382 galactic Aqr Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:25:48.34 -08:32:51.0 (user input) | T | P | (position from user input) J-Ks=0.269+/-0.036 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:25:48.34 -08:32:51.0: 13.28 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:25:48.34 -08:32:51.0: 13.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 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 10.3916 2461231.8916 11.84 22:28:41.12 -09:00:56.4
54.37624 -51.75550 galactic Aqr Second-epoch detections are separated by 0.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2621173838729693056 | 22:28:41.09 -09:00:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.617+/-0.033 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:28:41.12 -09:00:56.4: 12.82 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:28:41.12 -09:00:56.4: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.71 +/- 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
Gaia DR3 2621173838729693056,2461231.8916,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2621173838729693056 20260710.3916 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.88 22:27:38.67 -08:31:59.9
54.79886 -51.27629 galactic Aqr Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:38.67 -08:31:59.9 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.036 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:38.67 -08:31:59.9: 12.93 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:38.67 -08:31:59.9: 12.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.37 21:50:40.65 -13:16:44.7
41.84923 -45.65892 galactic Cap Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840404544720915072 | 21:50:40.57 -13:16:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.613+/-0.033 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:40.65 -13:16:44.7: 12.38 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:50:40.65 -13:16:44.7: 12.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 10.3916* 21 50 40.65 -13 16 44.7 11.4 U Cap 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 6840404544720915072,2461231.8916,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840404544720915072 20260710.3916 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.95 22:29:23.58 -08:56:25.1
54.63263 -51.86079 galactic Aqr Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:29:23.58 -08:56:25.1 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.031 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:23.58 -08:56:25.1: 12.79 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:23.58 -08:56:25.1: 12.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.26 22:29:01.39 -08:13:08.9
55.51973 -51.38630 galactic Aqr Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:29:01.39 -08:13:08.9 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.038 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:01.39 -08:13:08.9: 13.19 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:01.39 -08:13:08.9: 13.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.16 +/- 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,2461231.8916,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.20 21:49:57.42 -12:58:41.3
42.12900 -45.37098 galactic Cap Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843802031354835712 | 21:49:57.41 -12:58:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.567+/-0.032 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:57.42 -12:58:41.3: 12.36 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:57.42 -12:58:41.3: 12.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 10.3916* 21 49 57.42 -12 58 41.3 11.2 U Cap 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 6843802031354835712,2461231.8916,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843802031354835712 20260710.3916 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.09 21:54:38.31 -13:34:17.5
42.06319 -46.65456 galactic Cap Second-epoch detections are separated by 0.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840697972590832128 | 21:54:38.31 -13:34:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:38.31 -13:34:17.5: 12.09 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:54:38.31 -13:34:17.5: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 54 38.31 -13 34 17.5 11.1 U Cap 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 6840697972590832128,2461231.8916,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840697972590832128 20260710.3916 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.52 21:49:22.30 -12:49:33.0
42.23618 -45.17642 galactic Cap Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:22.30 -12:49:33.0 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.030 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:22.30 -12:49:33.0: 12.56 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:22.30 -12:49:33.0: 12.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.62 +/- 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!
TCP 2026 07 10.3916* 21 49 22.30 -12 49 33.0 11.5 U Cap 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,2461231.8916,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.69 21:52:58.83 -13:33:08.6
41.83844 -46.28204 galactic Cap Second-epoch detections are separated by 1.1" and 3.5 pix
The object was found in VSX 1" Gaia DR3 6840707460173969408
Type: ROT
# Max. Min./Amp. JD0 Period
12.660 G 12.680 G K
The object was found in astcheck.6290 1985 CA2 518 263 581 17.0 0 -0
NOTE: the measured brightness disagrees with the predicted asteroid brightness, but the matched variable star above likely accounts for this object.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:58.83 -13:33:08.6: 12.90 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:52:58.83 -13:33:08.6: 12.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 10.3916* 21 52 58.83 -13 33 08.6 11.7 U Cap 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 6840707460173969408,2461231.8916,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840707460173969408 20260710.3916 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 10.46 21:49:56.51 -13:12:40.2
41.82715 -45.46807 galactic Cap Second-epoch detections are separated by 0.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843411159266335232 | 21:49:56.49 -13:12:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.567+/-0.034 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:56.51 -13:12:40.2: 11.41 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:56.51 -13:12:40.2: 11.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 49 56.51 -13 12 40.2 10.5 U Cap 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 6843411159266335232,2461231.8916,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843411159266335232 20260710.3916 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.23 21:53:42.20 -13:18:51.0
42.25909 -46.33872 galactic Cap Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840720134622069120 | 21:53:42.13 -13:18:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.867+/-0.033 (M)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:42.20 -13:18:51.0: 12.36 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:42.20 -13:18:51.0: 12.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 42.20 -13 18 51.0 11.2 U Cap 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 6840720134622069120,2461231.8916,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840720134622069120 20260710.3916 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.59 21:56:07.56 -12:52:30.6
43.20632 -46.67890 galactic Cap Second-epoch detections are separated by 2.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840854721717094528 | 21:56:07.56 -12:52:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:07.56 -12:52:30.6: 12.53 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:56:07.56 -12:52:30.6: 12.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.54 +/- 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!
TCP 2026 07 10.3916* 21 56 07.56 -12 52 30.6 11.6 U Cap 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 6840854721717094528,2461231.8916,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840854721717094528 20260710.3916 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.23 22:25:48.03 -08:42:14.1
54.17401 -50.98800 galactic Aqr Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:25:48.03 -08:42:14.1 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:25:48.03 -08:42:14.1: 13.18 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:25:48.03 -08:42:14.1: 13.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.13 +/- 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,2461231.8916,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.54 21:56:46.32 -13:27:56.5
42.52864 -47.07749 galactic Cap Second-epoch detections are separated by 1.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840527342130527488 | 21:56:46.27 -13:27:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.672+/-0.033 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:46.32 -13:27:56.5: 12.50 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:56:46.32 -13:27:56.5: 12.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 56 46.32 -13 27 56.5 11.5 U Cap 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 6840527342130527488,2461231.8916,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840527342130527488 20260710.3916 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.34 22:33:35.86 -09:08:53.9
55.28226 -52.84236 galactic Aqr Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:33:35.86 -09:08:53.9 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.036 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:33:35.86 -09:08:53.9: 13.34 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:33:35.86 -09:08:53.9: 13.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.81 21:58:12.53 -13:39:00.6
42.50463 -47.47208 galactic Cap Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:12.53 -13:39:00.6 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:58:12.53 -13:39:00.6: 12.74 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:58:12.53 -13:39:00.6: 12.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 58 12.53 -13 39 00.6 11.8 U Cap 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,2461231.8916,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.84 22:28:46.19 -08:29:28.6
55.10082 -51.48524 galactic Aqr Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.12228 1985 TZ3 -381 -138 406 17.0 -0 -0
ATTENTION: measured mag 11.84 is 5.2 mag brighter than the predicted asteroid brightness 17.0 - the transient may be an unrelated new object!
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:28:46.19 -08:29:28.6: 12.90 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:28:46.19 -08:29:28.6: 12.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461231.8916,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3916 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.71 21:56:44.04 -13:00:39.1
43.12315 -46.87155 galactic Cap Second-epoch detections are separated by 0.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:44.04 -13:00:39.1 (user input) | T | P | (position from user input) J-Ks=0.734+/-0.029 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:44.04 -13:00:39.1: 12.73 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:56:44.04 -13:00:39.1: 12.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 10.3916* 21 56 44.04 -13 00 39.1 11.7 U Cap 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,2461231.8916,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.10 21:50:23.04 -13:30:08.7
41.51659 -45.68976 galactic Cap Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840391384941115136 | 21:50:23.00 -13:30:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.694+/-0.031 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:23.04 -13:30:08.7: 12.07 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:50:23.04 -13:30:08.7: 12.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 50 23.04 -13 30 08.7 11.1 U Cap 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 6840391384941115136,2461231.8916,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840391384941115136 20260710.3916 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.02 21:54:26.28 -13:18:30.6
42.37827 -46.49755 galactic Cap Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840741403300118656 | 21:54:26.26 -13:18:30.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.628+/-0.032 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:26.28 -13:18:30.6: 12.03 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:54:26.28 -13:18:30.6: 12.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 10.3916* 21 54 26.28 -13 18 30.6 11.0 U Cap 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 6840741403300118656,2461231.8916,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840741403300118656 20260710.3916 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.89 21:57:12.55 -13:57:19.3
41.94357 -47.38279 galactic Cap Second-epoch detections are separated by 2.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:12.55 -13:57:19.3 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.030 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:57:12.55 -13:57:19.3: 13.06 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:57:12.55 -13:57:19.3: 13.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 10.3916* 21 57 12.55 -13 57 19.3 11.9 U Cap 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,2461231.8916,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.19 21:53:18.30 -13:11:01.1
42.36891 -46.19495 galactic Cap Second-epoch detections are separated by 0.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840793045986880768 | 21:53:18.33 -13:11:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.268+/-0.033 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:18.30 -13:11:01.1: 12.03 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:18.30 -13:11:01.1: 12.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.07 +/- 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 10.3916* 21 53 18.30 -13 11 01.1 11.2 U Cap 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 6840793045986880768,2461231.8916,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840793045986880768 20260710.3916 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.42 21:53:35.20 -13:40:50.1
41.76123 -46.46990 galactic Cap Second-epoch detections are separated by 0.7" and 3.4 pix
The object was found in VSX 1" Gaia DR3 6840690172930225024
Type: ROT
# Max. Min./Amp. JD0 Period
12.240 G 12.260 G G
The object was not found in astcheck.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:35.20 -13:40:50.1: 12.29 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:35.20 -13:40:50.1: 12.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 35.20 -13 40 50.1 11.4 U Cap 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 6840690172930225024,2461231.8916,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840690172930225024 20260710.3916 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.51 21:58:24.53 -13:31:35.8
42.70055 -47.46276 galactic Cap Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840569948205654272 | 21:58:24.53 -13:31:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.521+/-0.029 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:58:24.53 -13:31:35.8: 12.52 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:58:24.53 -13:31:35.8: 12.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 58 24.53 -13 31 35.8 11.5 U Cap 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 6840569948205654272,2461231.8916,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840569948205654272 20260710.3916 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.29 21:49:43.17 -13:05:16.7
41.95244 -45.36623 galactic Cap Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843425105024996608 | 21:49:43.14 -13:05:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:43.17 -13:05:16.7: 12.28 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:43.17 -13:05:16.7: 12.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 49 43.17 -13 05 16.7 11.3 U Cap 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 6843425105024996608,2461231.8916,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843425105024996608 20260710.3916 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.76 22:27:36.45 -08:22:33.8
55.00034 -51.18199 galactic Aqr Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2621434560424461440 | 22:27:36.43 -08:22:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.424+/-0.035 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:36.45 -08:22:33.8: 12.71 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:36.45 -08:22:33.8: 12.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2621434560424461440,2461231.8916,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2621434560424461440 20260710.3916 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.68 21:56:01.10 -13:15:24.1
42.68863 -46.82184 galactic Cap Second-epoch detections are separated by 2.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:01.10 -13:15:24.1 (user input) | T | P | (position from user input) J-Ks=0.679+/-0.032 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:01.10 -13:15:24.1: 12.69 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:56:01.10 -13:15:24.1: 12.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 56 01.10 -13 15 24.1 11.7 U Cap 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,2461231.8916,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.27 21:49:43.84 -12:58:08.3
42.10682 -45.31730 galactic Cap Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843805123731267072 | 21:49:43.78 -12:58:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.562+/-0.031 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:43.84 -12:58:08.3: 12.29 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:43.84 -12:58:08.3: 12.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 49 43.84 -12 58 08.3 11.3 U Cap 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 6843805123731267072,2461231.8916,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843805123731267072 20260710.3916 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.28 22:29:14.12 -08:58:14.1
54.55713 -51.84474 galactic Aqr Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:29:14.12 -08:58:14.1 (user input) | T | P | (position from user input) J-Ks=0.573+/-0.030 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:14.12 -08:58:14.1: 13.21 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:14.12 -08:58:14.1: 13.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.06 21:54:42.11 -13:27:06.2
42.23044 -46.61712 galactic Cap Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840723089559573376 | 21:54:42.12 -13:27:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:42.11 -13:27:06.2: 11.99 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:54:42.11 -13:27:06.2: 12.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.01 +/- 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 10.3916* 21 54 42.11 -13 27 06.2 11.1 U Cap 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 6840723089559573376,2461231.8916,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840723089559573376 20260710.3916 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.25 21:53:55.50 -13:22:58.2
42.20288 -46.41694 galactic Cap Second-epoch detections are separated by 1.2" and 3.2 pix
The object was found in VSX 2" Gaia DR3 6840715981389078656
Type: ROT
# Max. Min./Amp. JD0 Period
12.110 G 12.140 G K
The object was not found in astcheck.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:55.50 -13:22:58.2: 12.28 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:55.50 -13:22:58.2: 12.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 55.50 -13 22 58.2 11.2 U Cap 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 6840715981389078656,2461231.8916,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840715981389078656 20260710.3916 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.27 22:29:20.65 -08:42:55.1
54.92605 -51.72723 galactic Aqr Second-epoch detections are separated by 0.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:29:20.65 -08:42:55.1 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.035 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:20.65 -08:42:55.1: 13.15 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:20.65 -08:42:55.1: 13.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.16 +/- 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,2461231.8916,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.39 21:49:56.17 -13:23:16.6
41.59834 -45.54248 galactic Cap Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843404351743080960 | 21:49:56.14 -13:23:16.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:56.17 -13:23:16.6: 12.52 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:56.17 -13:23:16.6: 12.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 49 56.17 -13 23 16.6 11.4 U Cap 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 6843404351743080960,2461231.8916,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843404351743080960 20260710.3916 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.35 22:31:37.19 -08:41:18.6
55.46685 -52.18099 galactic Aqr Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:31:37.19 -08:41:18.6 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.034 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:31:37.19 -08:41:18.6: 13.31 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:31:37.19 -08:41:18.6: 13.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461231.8916,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.04 21:53:55.27 -13:12:24.3
42.43258 -46.34017 galactic Cap Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840745354670026880 | 21:53:55.29 -13:12:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.031 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:55.27 -13:12:24.3: 12.00 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:55.27 -13:12:24.3: 11.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.99 +/- 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 10.3916* 21 53 55.27 -13 12 24.3 11.0 U Cap 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 6840745354670026880,2461231.8916,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840745354670026880 20260710.3916 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.89 22:33:22.42 -08:48:17.5
55.70344 -52.60584 galactic Aqr Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:33:22.42 -08:48:17.5 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.033 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:33:22.42 -08:48:17.5: 12.86 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:33:22.42 -08:48:17.5: 12.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.82 22:27:17.65 -08:21:17.3
54.96038 -51.10564 galactic Aqr Second-epoch detections are separated by 1.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:27:17.65 -08:21:17.3 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:17.65 -08:21:17.3: 12.87 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:27:17.65 -08:21:17.3: 12.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.34 21:58:12.00 -13:17:37.0
42.97824 -47.31605 galactic Cap Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840626405551270272 | 21:58:11.98 -13:17:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.401+/-0.029 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:58:12.00 -13:17:37.0: 12.26 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:58:12.00 -13:17:37.0: 12.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 58 12.00 -13 17 37.0 11.3 U Cap 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 6840626405551270272,2461231.8916,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840626405551270272 20260710.3916 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.26 21:53:35.95 -13:33:52.7
41.91535 -46.42325 galactic Cap Second-epoch detections are separated by 0.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840700760024979712 | 21:53:35.93 -13:33:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.629+/-0.042 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:35.95 -13:33:52.7: 12.25 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:35.95 -13:33:52.7: 12.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 35.95 -13 33 52.7 11.3 U Cap 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 6840700760024979712,2461231.8916,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840700760024979712 20260710.3916 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.32 21:50:58.24 -13:08:45.5
42.06509 -45.66611 galactic Cap Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843784890140864640 | 21:50:58.19 -13:08:44.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.031 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:58.24 -13:08:45.5: 12.24 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:50:58.24 -13:08:45.5: 12.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 50 58.24 -13 08 45.5 11.3 U Cap 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 6843784890140864640,2461231.8916,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843784890140864640 20260710.3916 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.05 21:52:12.10 -13:21:58.9
41.96428 -46.03131 galactic Cap Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840760545969773312 | 21:52:12.10 -13:21:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.033 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:12.10 -13:21:58.9: 11.98 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:52:12.10 -13:21:58.9: 12.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 10.3916* 21 52 12.10 -13 21 58.9 11.1 U Cap 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 6840760545969773312,2461231.8916,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840760545969773312 20260710.3916 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.45 21:53:58.49 -13:30:53.1
42.03746 -46.48447 galactic Cap Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840702095759433984 | 21:53:58.51 -13:30:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.259+/-0.032 (F)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:58.49 -13:30:53.1: 12.48 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:53:58.49 -13:30:53.1: 12.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 53 58.49 -13 30 53.1 11.4 U Cap 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 6840702095759433984,2461231.8916,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840702095759433984 20260710.3916 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.76 22:29:10.76 -08:23:13.5
55.33028 -51.51183 galactic Aqr Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.12228 1985 TZ3 -17 237 237 17.0 -0 -0
ATTENTION: measured mag 11.76 is 5.2 mag brighter than the predicted asteroid brightness 17.0 - the transient may be an unrelated new object!
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:10.76 -08:23:13.5: 12.67 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:29:10.76 -08:23:13.5: 12.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461231.8916,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3916 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.70 21:54:27.93 -13:25:29.0
42.23000 -46.55363 galactic Cap Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.6187-13.4208 | 21:54:27.93 -13:25:29.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.361+/-0.035 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:27.93 -13:25:29.0: 12.84 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:54:27.93 -13:25:29.0: 12.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 54 27.93 -13 25 29.0 11.7 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.6187-13.4208,2461231.8916,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.6187-13.4208 20260710.3916 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 11.21 21:54:48.99 -13:11:00.6
42.59992 -46.52653 galactic Cap Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6840748447046478976 | 21:54:49.01 -13:11:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.030 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:48.99 -13:11:00.6: 12.24 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:54:48.99 -13:11:00.6: 12.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 54 48.99 -13 11 00.6 11.2 U Cap 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 6840748447046478976,2461231.8916,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840748447046478976 20260710.3916 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.07 22:33:20.87 -09:00:23.2
55.42125 -52.71252 galactic Aqr Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:33:20.87 -09:00:23.2 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:33:20.87 -09:00:23.2: 13.01 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:33:20.87 -09:00:23.2: 12.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 10.96 21:49:05.11 -13:27:45.0
41.37651 -45.38699 galactic Cap Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.57073 2001 OB13 311 222 382 17.4 0 0
ATTENTION: measured mag 10.96 is 6.4 mag brighter than the predicted asteroid brightness 17.4 - the transient may be an unrelated new object!
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:05.11 -13:27:45.0: 11.97 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:05.11 -13:27:45.0: 12.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 10.3916* 21 49 05.11 -13 27 45.0 11.0 U Cap 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
VARIABLE_NAME,2461231.8916,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3916 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 10.66 21:49:44.83 -13:28:58.8
41.44760 -45.54138 galactic Cap Second-epoch detections are separated by 0.1" and 3.4 pix
The object was found in VSX 1" Gaia DR3 6840395095792870144
Type: ROT
# Max. Min./Amp. JD0 Period
11.570 G 11.610 G G
The object was not found in astcheck.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:44.83 -13:28:58.8: 11.59 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:44.83 -13:28:58.8: 11.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 49 44.83 -13 28 58.8 10.7 U Cap 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 6840395095792870144,2461231.8916,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6840395095792870144 20260710.3916 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 12.08 22:32:49.60 -08:53:11.6
55.46810 -52.53894 galactic Aqr Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:32:49.60 -08:53:11.6 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.035 (G)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:32:49.60 -08:53:11.6: 13.04 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 22:32:49.60 -08:53:11.6: 12.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8916,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3916 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3916 2461231.8916 10.59 21:49:39.91 -13:24:15.2
41.53721 -45.48981 galactic Cap Second-epoch detections are separated by 1.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6843398583602681472 | 21:49:39.87 -13:24:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.609+/-0.033 (K)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:39.91 -13:24:15.2: 11.56 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits at 21:49:39.91 -13:24:15.2: 11.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3916* 21 49 39.91 -13 24 15.2 10.6 U Cap 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 6843398583602681472,2461231.8916,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6843398583602681472 20260710.3916 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.89957081 17.05.2026 09:35:12.918 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
First image: 2461177.89957081 17.05.2026 09:35:12.918 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Last image: 2461231.89185281 10.07.2026 09:24:06.083 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 4 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): 2832
Objects passed selection criteria: 2829
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 2016
Average stars matched: 1989.5 (98.6855 %)
Memory usage VmPeak: 110016 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 06:37:51 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: 2461177.89957081 17.05.2026 09:35:12.918 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
First image: 2461177.89957081 17.05.2026 09:35:12.918 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Last image: 2461231.89185281 10.07.2026 09:24:06.083 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 131
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.81
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: 13 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): 19787
Objects passed selection criteria: 19731
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 14354
Average stars matched: 13967.5 (97.3074 %)
Memory usage VmPeak: 126520 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 06:40:00 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/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.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/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.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: 2461231.89138807
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_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:05.881 -09:59:58.55 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/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_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.902 -09:59:59.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:05.881 -09:59:58.55
Second-epoch image center 22:17:08.902 -09:59:59.02
Angular distance between the image centers 0.0124 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.262 -10:00:18.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:05.881 -09:59:58.55
Second-epoch image center 22:17:09.262 -10:00:18.76
Angular distance between the image centers 0.0150 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 22:17:08.902 -09:59:59.02
Second-epoch second image center 22:17:09.262 -10:00:18.76
Angular distance between the image centers 0.00568 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/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.JCgWzB2sAp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits &> /tmp/tmp.uBlhUEGq3H
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits &> /tmp/tmp.AXzstbxhfO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits &> /tmp/tmp.gHgPVRpqzc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat' -> 'wcsmag.cat'
Read 4507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 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 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 deg
Loaded 5486 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): 3392 out of 3444 total matches.
Matched with Tycho-2 3444 out of 4507 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.442350
a=0.000000 b=1.000000 c=22.442350
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 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 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 deg
Loaded 5486 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): 3392 out of 3444 total matches.
Matched with Tycho-2 3444 out of 4507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (aperture=6.1)
Read 3781 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2567 to 342.4099 deg, Dec -15.2423 to -4.6696 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 326.2567 to 342.4099 deg, Dec -15.2423 to -4.6696 deg
Loaded 5072 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): 3002 out of 3043 total matches.
Matched with Tycho-2 3043 out of 3781 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
2.3 pix Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
2.3 pix wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
Limiting magnitude estimates:
14.4 mag. Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
14.1 mag. Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
11.9 mag. fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
12.3 mag. fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
All-image limiting magnitude estimate: 11.9 (SNR ) 9.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JCgWzB2sAp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=252, bad_region=782, passed=4507
Got 4507 stars (including 3517 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 4507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 3759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 3757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 3757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 870 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=870 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.275 sigma_q2_arcsec=0.293 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.289 n_q1=313 n_q2=125 n_q3=313 n_q4=119 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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.uBlhUEGq3H (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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=273, bad_region=858, passed=3781
Got 3781 stars (including 2706 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat
util/solve_plate_with_UCAC5 got 3781 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 2999 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 2997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 2997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits N_match=882 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.365 sigma_q3_arcsec=0.507 sigma_q4_arcsec=0.434 n_q1=308 n_q2=146 n_q3=296 n_q4=132 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits -region wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.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.AXzstbxhfO (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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=72, bad_region=384, passed=1058
Got 1058 stars (including 632 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 1058 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 374 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 525 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 524 matched stars entering correct_measured_positions(), 483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 524 matched stars entering correct_measured_positions(), 656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 374 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 525 matched stars entering correct_measured_positions(), 660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 525 matched stars entering correct_measured_positions(), 660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 525 stars left (next iteration limit 576)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits N_match=525 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.396 sigma_q3_arcsec=0.542 sigma_q4_arcsec=0.463 n_q1=167 n_q2=106 n_q3=123 n_q4=129 worst_quadrant_to_overall_ratio=1.168
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.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.gHgPVRpqzc (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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.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_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=79, bad_region=415, passed=1185
Got 1185 stars (including 724 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat
util/solve_plate_with_UCAC5 got 1185 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 606 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 605 matched stars entering correct_measured_positions(), 576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 605 matched stars entering correct_measured_positions(), 769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 606 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 605 matched stars entering correct_measured_positions(), 769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 605 matched stars entering correct_measured_positions(), 769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 605 stars left (next iteration limit 665)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits N_match=605 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.421 sigma_q3_arcsec=0.532 sigma_q4_arcsec=0.446 n_q1=204 n_q2=112 n_q3=153 n_q4=136 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.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=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits sigma_overall=0.274 worst_q_ratio=1.070
ref2=Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits sigma_overall=0.424 worst_q_ratio=1.198
new1=fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits sigma_overall=0.464 worst_q_ratio=1.168
new2=fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits sigma_overall=0.466 worst_q_ratio=1.142
reference average sigma_overall=0.349 worst_q_ratio=1.134
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447_astrometric_residuals.png (870 matched stars from wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402_astrometric_residuals.png (882 matched stars from wcs_Aqr-04-Q2b1x1_2026-05-28_05-31-10_20.00sec_5.00C_LIGHT_0402.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406_astrometric_residuals.png (525 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407_astrometric_residuals.png (605 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-23-25_20.00sec_4.90C_LIGHT_0406.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Aqr-04-Q2b1x1_045304_TTUQ2b1x1_2555478_DdDrFQOT/wcs_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
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Considering the candidate 20106_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 20106_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 31523_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 31523_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 31525_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 31525_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 31530_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 31530_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 31532_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 31532_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 26318_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26318_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03769_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03769_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 26189_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26189_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 19721_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 19721_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
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Considering the candidate 26990_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26990_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 04054_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 04054_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03290_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03290_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 19982_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 19982_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02589_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02589_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03805_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03805_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02482_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02482_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03814_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03814_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 26615_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26615_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03301_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03301_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 19915_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 19915_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02720_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02720_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 27220_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 27220_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 20496_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20496_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03389_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03389_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 27330_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 27330_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03795_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03795_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 04267_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 04267_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 21079_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 21079_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 26248_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26248_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 20814_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20814_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 19967_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 19967_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 20823_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20823_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 27018_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 27018_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03008_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03008_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18306_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 18306_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18063_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 18063_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
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Considering the candidate 26403_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26403_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19770_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 19770_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26634_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 26634_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03633_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03633_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02566_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02566_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03935_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03935_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02549_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02549_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03129_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03129_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03083_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03083_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04154_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 04154_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20109_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20109_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18561_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 18561_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02909_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02909_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20983_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20983_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02567_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02567_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19921_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 19921_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26855_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 26855_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19875_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 19875_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03875_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03875_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02521_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02521_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03139_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03139_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01921_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 01921_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03356_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03356_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02316_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02316_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02848_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02848_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03393_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03393_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26788_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26788_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03324_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03324_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03646_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03646_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20665_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20665_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02836_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02836_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24999_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 24999_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02947_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02947_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27308_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 27308_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02758_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02758_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 20030_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20030_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03332_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03332_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 20154_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20154_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 19829_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 19829_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03331_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03331_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02537_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02537_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 03322_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03322_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 27029_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 27029_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
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Considering the candidate 02914_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02914_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02679_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02679_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 26706_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 26706_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02900_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02900_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03408_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 03408_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 18325_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 18325_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02548_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02548_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
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Considering the candidate 02522_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02522_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19885_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 19885_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
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Considering the candidate 20160_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 20160_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02702_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
Preparing report for the candidate 02702_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20513_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407
The candidate 20513_fd_Aqr-04-Q2b1x1_2026-07-10_04-24-06_20.00sec_4.90C_LIGHT_0407 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 157s
Prepared the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:57:12.55 -13:57:19.3
21:53:35.20 -13:40:50.1
21:53:15.99 -13:35:35.3
21:50:23.04 -13:30:08.7
21:49:44.83 -13:28:58.8
21:53:35.95 -13:33:52.7
21:49:05.11 -13:27:45.0
21:52:58.83 -13:33:08.6
21:54:38.31 -13:34:17.5
21:58:12.53 -13:39:00.6
21:57:48.08 -13:37:59.8
21:53:58.49 -13:30:53.1
21:49:39.91 -13:24:15.2
21:50:16.80 -13:24:51.9
21:49:56.17 -13:23:16.6
21:54:42.11 -13:27:06.2
21:58:24.53 -13:31:35.8
21:54:27.93 -13:25:29.0
21:56:46.32 -13:27:56.5
21:52:12.10 -13:21:58.9
21:53:55.50 -13:22:58.2
21:50:40.65 -13:16:44.7
21:53:42.20 -13:18:51.0
21:49:56.51 -13:12:40.2
21:54:26.28 -13:18:30.6
21:53:24.58 -13:13:09.4
21:53:18.83 -13:12:29.0
21:50:58.24 -13:08:45.5
21:56:01.10 -13:15:24.1
21:58:12.00 -13:17:37.0
21:53:55.27 -13:12:24.3
21:53:18.30 -13:11:01.1
21:54:47.77 -13:11:56.2
21:49:43.17 -13:05:16.7
21:54:48.99 -13:11:00.6
21:49:57.42 -12:58:41.3
21:49:43.84 -12:58:08.3
21:55:22.75 -13:01:45.4
21:51:15.10 -12:55:38.4
21:56:19.64 -13:01:44.6
21:49:51.83 -12:53:19.3
21:56:44.04 -13:00:39.1
21:49:22.30 -12:49:33.0
21:51:33.47 -12:49:17.4
21:56:07.56 -12:52:30.6
21:50:06.34 -12:42:20.0
22:29:23.58 -08:56:25.1
22:33:20.87 -09:00:23.2
22:27:17.65 -08:21:17.3
22:30:17.73 -08:29:52.2
22:28:46.19 -08:29:28.6
22:25:48.34 -08:32:51.0
22:26:42.91 -08:34:16.1
22:31:37.19 -08:41:18.6
22:25:48.03 -08:42:14.1
22:33:22.42 -08:48:17.5
22:32:49.60 -08:53:11.6
22:29:50.57 -08:53:49.1
22:29:14.12 -08:58:14.1
22:27:57.51 -09:01:07.5
22:28:41.12 -09:00:56.4
22:33:35.86 -09:08:53.9
22:28:11.01 -09:06:56.3
22:25:54.36 -08:03:04.4
22:25:54.60 -08:05:12.2
22:26:36.54 -08:06:48.5
22:29:01.39 -08:13:08.9
22:27:16.71 -08:18:07.5
22:29:10.76 -08:23:13.5
22:27:36.45 -08:22:33.8
22:31:07.94 -08:34:00.8
22:27:38.67 -08:31:59.9
22:27:26.84 -08:39:16.6
22:29:20.65 -08:42:55.1
22:27:54.04 -08:41:42.4
22:29:33.33 -11:22:31.9
########### Completed Aqr-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
22:29:33.33 -11:22:31.9
22:26:36.54 -08:06:48.5
21:55:22.75 -13:01:45.4
22:25:54.36 -08:03:04.4
22:31:07.94 -08:34:00.8
21:51:33.47 -12:49:17.4
21:53:24.58 -13:13:09.4
22:26:42.91 -08:34:16.1
21:57:48.08 -13:37:59.8
21:56:19.64 -13:01:44.6
21:53:15.99 -13:35:35.3
21:49:51.83 -12:53:19.3
22:27:16.71 -08:18:07.5
21:53:18.83 -13:12:29.0
22:30:17.73 -08:29:52.2
21:50:16.80 -13:24:51.9
22:27:26.84 -08:39:16.6
22:29:50.57 -08:53:49.1
21:54:47.77 -13:11:56.2
22:27:54.04 -08:41:42.4
21:51:15.10 -12:55:38.4
21:50:06.34 -12:42:20.0
22:28:11.01 -09:06:56.3
22:25:54.60 -08:05:12.2
22:27:57.51 -09:01:07.5
22:25:48.34 -08:32:51.0
22:28:41.12 -09:00:56.4
22:27:38.67 -08:31:59.9
21:50:40.65 -13:16:44.7
22:29:23.58 -08:56:25.1
22:29:01.39 -08:13:08.9
21:49:57.42 -12:58:41.3
21:54:38.31 -13:34:17.5
21:49:22.30 -12:49:33.0
21:52:58.83 -13:33:08.6
21:49:56.51 -13:12:40.2
21:53:42.20 -13:18:51.0
21:56:07.56 -12:52:30.6
22:25:48.03 -08:42:14.1
21:56:46.32 -13:27:56.5
22:33:35.86 -09:08:53.9
21:58:12.53 -13:39:00.6
22:28:46.19 -08:29:28.6
21:56:44.04 -13:00:39.1
21:50:23.04 -13:30:08.7
21:54:26.28 -13:18:30.6
21:57:12.55 -13:57:19.3
21:53:18.30 -13:11:01.1
21:53:35.20 -13:40:50.1
21:58:24.53 -13:31:35.8
21:49:43.17 -13:05:16.7
22:27:36.45 -08:22:33.8
21:56:01.10 -13:15:24.1
21:49:43.84 -12:58:08.3
22:29:14.12 -08:58:14.1
21:54:42.11 -13:27:06.2
21:53:55.50 -13:22:58.2
22:29:20.65 -08:42:55.1
21:49:56.17 -13:23:16.6
22:31:37.19 -08:41:18.6
21:53:55.27 -13:12:24.3
22:33:22.42 -08:48:17.5
22:27:17.65 -08:21:17.3
21:58:12.00 -13:17:37.0
21:53:35.95 -13:33:52.7
21:50:58.24 -13:08:45.5
21:52:12.10 -13:21:58.9
21:53:58.49 -13:30:53.1
22:29:10.76 -08:23:13.5
21:54:27.93 -13:25:29.0
21:54:48.99 -13:11:00.6
22:33:20.87 -09:00:23.2
21:49:05.11 -13:27:45.0
21:49:44.83 -13:28:58.8
22:32:49.60 -08:53:11.6
21:49:39.91 -13:24:15.2
###################################################################################
22:29:33.33 -11:22:31.9 -- asteroid (will NOT add it to exclusion list)
22:26:36.54 -08:06:48.5 -- not an asteroid (will add it to exclusion list)
21:55:22.75 -13:01:45.4 -- not an asteroid (will add it to exclusion list)
22:25:54.36 -08:03:04.4 -- not an asteroid (will add it to exclusion list)
22:31:07.94 -08:34:00.8 -- not an asteroid (will add it to exclusion list)
21:51:33.47 -12:49:17.4 -- not an asteroid (will add it to exclusion list)
21:53:24.58 -13:13:09.4 -- not an asteroid (will add it to exclusion list)
22:26:42.91 -08:34:16.1 -- not an asteroid (will add it to exclusion list)
21:57:48.08 -13:37:59.8 -- not an asteroid (will add it to exclusion list)
21:56:19.64 -13:01:44.6 -- not an asteroid (will add it to exclusion list)
21:53:15.99 -13:35:35.3 -- not an asteroid (will add it to exclusion list)
21:49:51.83 -12:53:19.3 -- not an asteroid (will add it to exclusion list)
22:27:16.71 -08:18:07.5 -- not an asteroid (will add it to exclusion list)
21:53:18.83 -13:12:29.0 -- not an asteroid (will add it to exclusion list)
22:30:17.73 -08:29:52.2 -- not an asteroid (will add it to exclusion list)
21:50:16.80 -13:24:51.9 -- not an asteroid (will add it to exclusion list)
22:27:26.84 -08:39:16.6 -- not an asteroid (will add it to exclusion list)
22:29:50.57 -08:53:49.1 -- not an asteroid (will add it to exclusion list)
21:54:47.77 -13:11:56.2 -- not an asteroid (will add it to exclusion list)
22:27:54.04 -08:41:42.4 -- not an asteroid (will add it to exclusion list)
21:51:15.10 -12:55:38.4 -- not an asteroid (will add it to exclusion list)
21:50:06.34 -12:42:20.0 -- not an asteroid (will add it to exclusion list)
22:28:11.01 -09:06:56.3 -- not an asteroid (will add it to exclusion list)
22:25:54.60 -08:05:12.2 -- not an asteroid (will add it to exclusion list)
22:27:57.51 -09:01:07.5 -- not an asteroid (will add it to exclusion list)
22:25:48.34 -08:32:51.0 -- not an asteroid (will add it to exclusion list)
22:28:41.12 -09:00:56.4 -- not an asteroid (will add it to exclusion list)
22:27:38.67 -08:31:59.9 -- not an asteroid (will add it to exclusion list)
21:50:40.65 -13:16:44.7 -- not an asteroid (will add it to exclusion list)
22:29:23.58 -08:56:25.1 -- not an asteroid (will add it to exclusion list)
22:29:01.39 -08:13:08.9 -- not an asteroid (will add it to exclusion list)
21:49:57.42 -12:58:41.3 -- not an asteroid (will add it to exclusion list)
21:54:38.31 -13:34:17.5 -- not an asteroid (will add it to exclusion list)
21:49:22.30 -12:49:33.0 -- not an asteroid (will add it to exclusion list)
21:52:58.83 -13:33:08.6 -- asteroid (will NOT add it to exclusion list)
21:49:56.51 -13:12:40.2 -- not an asteroid (will add it to exclusion list)
21:53:42.20 -13:18:51.0 -- not an asteroid (will add it to exclusion list)
21:56:07.56 -12:52:30.6 -- not an asteroid (will add it to exclusion list)
22:25:48.03 -08:42:14.1 -- not an asteroid (will add it to exclusion list)
21:56:46.32 -13:27:56.5 -- not an asteroid (will add it to exclusion list)
22:33:35.86 -09:08:53.9 -- not an asteroid (will add it to exclusion list)
21:58:12.53 -13:39:00.6 -- not an asteroid (will add it to exclusion list)
22:28:46.19 -08:29:28.6 -- asteroid (will NOT add it to exclusion list)
21:56:44.04 -13:00:39.1 -- not an asteroid (will add it to exclusion list)
21:50:23.04 -13:30:08.7 -- not an asteroid (will add it to exclusion list)
21:54:26.28 -13:18:30.6 -- not an asteroid (will add it to exclusion list)
21:57:12.55 -13:57:19.3 -- not an asteroid (will add it to exclusion list)
21:53:18.30 -13:11:01.1 -- not an asteroid (will add it to exclusion list)
21:53:35.20 -13:40:50.1 -- not an asteroid (will add it to exclusion list)
21:58:24.53 -13:31:35.8 -- not an asteroid (will add it to exclusion list)
21:49:43.17 -13:05:16.7 -- not an asteroid (will add it to exclusion list)
22:27:36.45 -08:22:33.8 -- not an asteroid (will add it to exclusion list)
21:56:01.10 -13:15:24.1 -- not an asteroid (will add it to exclusion list)
21:49:43.84 -12:58:08.3 -- not an asteroid (will add it to exclusion list)
22:29:14.12 -08:58:14.1 -- not an asteroid (will add it to exclusion list)
21:54:42.11 -13:27:06.2 -- not an asteroid (will add it to exclusion list)
21:53:55.50 -13:22:58.2 -- not an asteroid (will add it to exclusion list)
22:29:20.65 -08:42:55.1 -- not an asteroid (will add it to exclusion list)
21:49:56.17 -13:23:16.6 -- not an asteroid (will add it to exclusion list)
22:31:37.19 -08:41:18.6 -- not an asteroid (will add it to exclusion list)
21:53:55.27 -13:12:24.3 -- not an asteroid (will add it to exclusion list)
22:33:22.42 -08:48:17.5 -- not an asteroid (will add it to exclusion list)
22:27:17.65 -08:21:17.3 -- not an asteroid (will add it to exclusion list)
21:58:12.00 -13:17:37.0 -- not an asteroid (will add it to exclusion list)
21:53:35.95 -13:33:52.7 -- not an asteroid (will add it to exclusion list)
21:50:58.24 -13:08:45.5 -- not an asteroid (will add it to exclusion list)
21:52:12.10 -13:21:58.9 -- not an asteroid (will add it to exclusion list)
21:53:58.49 -13:30:53.1 -- not an asteroid (will add it to exclusion list)
22:29:10.76 -08:23:13.5 -- asteroid (will NOT add it to exclusion list)
21:54:27.93 -13:25:29.0 -- not an asteroid (will add it to exclusion list)
21:54:48.99 -13:11:00.6 -- not an asteroid (will add it to exclusion list)
22:33:20.87 -09:00:23.2 -- not an asteroid (will add it to exclusion list)
21:49:05.11 -13:27:45.0 -- asteroid (will NOT add it to exclusion list)
21:49:44.83 -13:28:58.8 -- not an asteroid (will add it to exclusion list)
22:32:49.60 -08:53:11.6 -- not an asteroid (will add it to exclusion list)
21:49:39.91 -13:24:15.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:49:22.30 -12:49:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:39.91 -13:24:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:43.17 -13:05:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:43.84 -12:58:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:44.83 -13:28:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:51.83 -12:53:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:56.17 -13:23:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:56.51 -13:12:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:57.42 -12:58:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:06.34 -12:42:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:16.80 -13:24:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:23.04 -13:30:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:40.65 -13:16:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:58.24 -13:08:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:15.10 -12:55:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:33.47 -12:49:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:12.10 -13:21:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:15.99 -13:35:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:18.30 -13:11:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:18.83 -13:12:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:24.58 -13:13:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:35.20 -13:40:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:35.95 -13:33:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:42.20 -13:18:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:55.27 -13:12:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:55.50 -13:22:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:58.49 -13:30:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:26.28 -13:18:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:27.93 -13:25:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:38.31 -13:34:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:42.11 -13:27:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:47.77 -13:11:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:48.99 -13:11:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:22.75 -13:01:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:01.10 -13:15:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:07.56 -12:52:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:19.64 -13:01:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:44.04 -13:00:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:46.32 -13:27:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:12.55 -13:57:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:48.08 -13:37:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:12.00 -13:17:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:12.53 -13:39:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:24.53 -13:31:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:48.03 -08:42:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:48.34 -08:32:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:54.36 -08:03:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:54.60 -08:05:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:36.54 -08:06:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:42.91 -08:34:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:16.71 -08:18:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:17.65 -08:21:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:26.84 -08:39:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:36.45 -08:22:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:38.67 -08:31:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:54.04 -08:41:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:57.51 -09:01:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:11.01 -09:06:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:41.12 -09:00:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:01.39 -08:13:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:14.12 -08:58:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:20.65 -08:42:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:23.58 -08:56:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:50.57 -08:53:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:30:17.73 -08:29:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:07.94 -08:34:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:37.19 -08:41:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:32:49.60 -08:53:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:33:20.87 -09:00:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:33:22.42 -08:48:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:33:35.86 -09:08:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:49:22.30 -12:49:33.0 -- not a known variable star
21:49:39.91 -13:24:15.2 -- not a known variable star
21:49:43.17 -13:05:16.7 -- not a known variable star
21:49:43.84 -12:58:08.3 -- not a known variable star
21:49:44.83 -13:28:58.8 -- a known variable star
21:49:51.83 -12:53:19.3 -- not a known variable star
21:49:56.17 -13:23:16.6 -- not a known variable star
21:49:56.51 -13:12:40.2 -- not a known variable star
21:49:57.42 -12:58:41.3 -- not a known variable star
21:50:06.34 -12:42:20.0 -- not a known variable star
21:50:16.80 -13:24:51.9 -- not a known variable star
21:50:23.04 -13:30:08.7 -- not a known variable star
21:50:40.65 -13:16:44.7 -- not a known variable star
21:50:58.24 -13:08:45.5 -- not a known variable star
21:51:15.10 -12:55:38.4 -- not a known variable star
21:51:33.47 -12:49:17.4 -- not a known variable star
21:52:12.10 -13:21:58.9 -- not a known variable star
21:53:15.99 -13:35:35.3 -- not a known variable star
21:53:18.30 -13:11:01.1 -- not a known variable star
21:53:18.83 -13:12:29.0 -- not a known variable star
21:53:24.58 -13:13:09.4 -- not a known variable star
21:53:35.20 -13:40:50.1 -- a known variable star
21:53:35.95 -13:33:52.7 -- not a known variable star
21:53:42.20 -13:18:51.0 -- not a known variable star
21:53:55.27 -13:12:24.3 -- not a known variable star
21:53:55.50 -13:22:58.2 -- a known variable star
21:53:58.49 -13:30:53.1 -- not a known variable star
21:54:26.28 -13:18:30.6 -- not a known variable star
21:54:27.93 -13:25:29.0 -- not a known variable star
21:54:38.31 -13:34:17.5 -- not a known variable star
21:54:42.11 -13:27:06.2 -- not a known variable star
21:54:47.77 -13:11:56.2 -- not a known variable star
21:54:48.99 -13:11:00.6 -- not a known variable star
21:55:22.75 -13:01:45.4 -- not a known variable star
21:56:01.10 -13:15:24.1 -- not a known variable star
21:56:07.56 -12:52:30.6 -- not a known variable star
21:56:19.64 -13:01:44.6 -- not a known variable star
21:56:44.04 -13:00:39.1 -- not a known variable star
21:56:46.32 -13:27:56.5 -- not a known variable star
21:57:12.55 -13:57:19.3 -- not a known variable star
21:57:48.08 -13:37:59.8 -- not a known variable star
21:58:12.00 -13:17:37.0 -- not a known variable star
21:58:12.53 -13:39:00.6 -- not a known variable star
21:58:24.53 -13:31:35.8 -- not a known variable star
22:25:48.03 -08:42:14.1 -- not a known variable star
22:25:48.34 -08:32:51.0 -- not a known variable star
22:25:54.36 -08:03:04.4 -- not a known variable star
22:25:54.60 -08:05:12.2 -- not a known variable star
22:26:36.54 -08:06:48.5 -- not a known variable star
22:26:42.91 -08:34:16.1 -- not a known variable star
22:27:16.71 -08:18:07.5 -- not a known variable star
22:27:17.65 -08:21:17.3 -- not a known variable star
22:27:26.84 -08:39:16.6 -- not a known variable star
22:27:36.45 -08:22:33.8 -- not a known variable star
22:27:38.67 -08:31:59.9 -- not a known variable star
22:27:54.04 -08:41:42.4 -- not a known variable star
22:27:57.51 -09:01:07.5 -- not a known variable star
22:28:11.01 -09:06:56.3 -- not a known variable star
22:28:41.12 -09:00:56.4 -- not a known variable star
22:29:01.39 -08:13:08.9 -- not a known variable star
22:29:14.12 -08:58:14.1 -- not a known variable star
22:29:20.65 -08:42:55.1 -- not a known variable star
22:29:23.58 -08:56:25.1 -- not a known variable star
22:29:50.57 -08:53:49.1 -- not a known variable star
22:30:17.73 -08:29:52.2 -- not a known variable star
22:31:07.94 -08:34:00.8 -- not a known variable star
22:31:37.19 -08:41:18.6 -- not a known variable star
22:32:49.60 -08:53:11.6 -- not a known variable star
22:33:20.87 -09:00:23.2 -- not a known variable star
22:33:22.42 -08:48:17.5 -- not a known variable star
22:33:35.86 -09:08:53.9 -- not a known variable star
Found 68 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
71 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 71 (excluding asteroids and hot pixels, 68 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)2461231.89138807 -observatory V36
07:32:10.44 +17:07:55.6 Mercury (5.1mag)
10:11:49.17 +12:39:55.4 Venus (-4.1mag)
04:24:17.61 +21:25:31.0 Mars (1.3mag)
08:16:42.81 +20:11:22.0 Jupiter (-1.8mag)
00:55:51.18 +03:20:29.8 Saturn (0.7mag)
04:07:14.51 +20:45:04.7 Uranus (5.8mag)
00:17:01.49 +00:20:41.0 Neptune (7.8mag)
20:30:54.71 -23:18:01.7 Pluto (14.4mag)
03:14:14.59 +22:35:44.6 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 06:37 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.89138807:
08:16:49.98 +20:10:56.8 Io (6.1mag)
08:16:46.38 +20:11:10.5 Europa (6.3mag)
08:17:00.02 +20:10:19.6 Ganymede (5.6mag)
08:17:10.61 +20:09:39.2 Callisto (6.8mag)
08:15:14.19 +19:55:32.6 Himalia (15.7mag)
08:16:43.19 +20:11:21.4 Thebe (16.6mag)
08:14:35.51 +20:00:01.6 Elara (17.6mag)
08:20:15.11 +20:05:30.8 Pasiphae (17.8mag)
08:21:40.52 +20:16:27.4 Carme (19.0mag)
00:55:41.14 +03:20:20.2 Titan (8.5mag)
00:55:45.93 +03:20:32.1 Rhea (9.8mag)
00:55:20.41 +03:19:38.2 Iapetus (11.2mag)
00:56:00.26 +03:20:49.2 Hyperion (14.5mag)
00:55:51.84 +03:17:43.2 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 06:37 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.89138807:
17:46:01.95 -32:57:35.6 JWST
16:20:56.28 +47:29:15.9 Chandra
04:58:04.27 +48:28:21.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 06:37 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.89138807 -observatory V36
02:36:19.58 +14:25:59.2 17.9mag P/1996 R2 (Lagerkvist)
18:17:54.47 -34:21:49.3 13.7mag P/2010 H2 (Vales)
06:25:42.89 -68:08:25.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:49.21 +32:26:51.5 17.6mag C/2017 K2 (PANSTARRS)
17:03:06.26 +16:02:53.7 18.0mag C/2021 G2 (ATLAS)
01:48:01.93 +08:18:05.9 15.4mag P/2021 N1 (ZTF)
22:59:30.45 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:26.72 +26:55:33.6 16.7mag C/2022 N2 (PANSTARRS)
09:55:33.00 +29:46:44.8 16.8mag C/2022 QE78 (ATLAS)
09:09:45.66 +05:00:00.0 17.8mag C/2022 R6 (PANSTARRS)
18:07:11.61 +21:17:32.5 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:34.97 -11:23:19.1 17.7mag P/2023 B1 (PANSTARRS)
21:49:11.19 +67:37:16.2 17.8mag C/2023 H5 (Lemmon)
16:30:48.37 -10:04:56.5 13.9mag C/2023 R1 (PANSTARRS)
08:00:43.19 +65:42:38.0 17.9mag C/2024 A1 (ATLAS)
07:32:52.04 +30:00:19.5 14.6mag C/2024 E1 (Wierzchos)
15:16:18.40 +15:19:45.9 17.5mag C/2024 G6 (ATLAS)
19:41:15.53 +39:24:03.2 13.8mag C/2024 J3 (ATLAS)
21:47:32.51 +46:00:33.5 17.8mag C/2024 R4 (PANSTARRS)
04:49:40.62 -13:47:38.7 15.7mag C/2024 T5 (ATLAS)
06:34:36.39 +29:03:47.9 18.0mag C/2025 J1 (Borisov)
07:14:22.09 -12:53:35.3 16.5mag C/2025 R3 (PANSTARRS)
09:56:08.27 +22:26:06.6 17.6mag C/2025 V2 (Rankin)
12:44:37.81 +03:56:10.2 17.1mag C/2025 Y1 (ATLAS)
16:51:50.32 +79:07:15.9 17.4mag C/2026 A2 (Bok)
02:46:19.11 +45:14:30.2 16.7mag C/2026 B2 (Sun-Gao)
11:25:32.19 +04:33:04.5 16.9mag A/2026 E1
21:19:05.66 -15:05:25.0 7.3mag 10P/Tempel
11:13:28.41 -01:53:19.8 16.1mag 29P/Schwassmann-Wachmann
04:00:13.76 +29:33:27.2 17.8mag 47P/Ashbrook-Jackson
10:08:09.57 +13:59:56.1 17.0mag 63P/Wild
00:48:22.77 -05:05:33.5 15.5mag 65P/Gunn
08:27:04.61 +34:13:01.4 17.9mag 76P/West-Kohoutek-Ikemura
04:27:29.61 +20:10:51.5 13.7mag 78P/Gehrels
02:22:23.89 +10:36:54.3 16.2mag 88P/Howell
06:35:38.90 +30:31:57.6 15.7mag 93P/Lovas
04:21:07.59 +31:07:29.6 16.9mag 114P/Wiseman-Skiff
08:08:47.46 +30:41:57.3 15.2mag 123P/West-Hartley
10:48:12.31 +01:10:15.4 16.8mag 124P/Mrkos
04:51:47.49 +20:48:51.1 16.2mag 128P/Shoemaker-Holt
05:36:19.80 +19:42:49.8 17.8mag 131P/Mueller
00:01:33.36 +02:56:12.6 17.9mag 139P/Vaisala-Oterma
07:13:42.51 +17:00:44.5 15.5mag 141P-D/Machholz
03:16:51.97 -21:06:09.7 15.5mag 161P/Hartley-IRAS
05:33:12.30 +33:57:26.5 15.3mag 162P/SidingSpring
19:04:22.31 +15:06:21.3 14.7mag 169P/NEAT
01:41:07.42 +07:36:11.6 17.7mag 220P/McNaught
16:35:57.73 -08:23:12.5 17.0mag 235P/LINEAR
08:45:22.14 +33:17:45.2 17.9mag 240P/NEAT
20:42:09.33 -49:34:45.6 17.8mag 259P/Garradd
01:59:24.91 +12:06:47.4 15.7mag 260P/McNaught
05:37:20.71 +36:50:46.6 17.4mag 295P/LINEAR
15:06:36.64 +06:03:12.4 17.6mag 391P/Kowalski
08:34:38.34 +19:40:30.7 17.9mag 450P/LONEOS
07:51:49.72 +39:12:46.7 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 06:37 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
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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 06:37 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:03:23.326 +12:49:15.53 AT 2026sqk 2026-07-06.95 17.816
02:23:45.306 -56:30:54.13 AT 2026sqj 2026-07-07.14 18.706
20:05:32.749 -40:04:20.18 AT 2026sqi 2026-07-07.00 19.025
13:27:09.068 +62:50:19.22 AT 2026sqh 2026-07-06.32 19.347
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
-rw-r--r-- 1 apache apache 30K Jul 10 06:37 tns_transients_list.txt
