This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9
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 10.3767 2461231.8767 12.02 02:53:08.81 +20:33:20.9
157.79662 -33.94849 galactic Ari Second-epoch detections are separated by 1.7" and 9.3 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 | 02:53:08.81 +20:33:20.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.715+/-0.033 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:08.81 +20:33:20.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:08.81 +20:33:20.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 53 08.81 +20 33 20.9 12.0 U Ari 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,2461231.8767,12.02,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.95 02:33:16.64 +20:21:30.8
153.01941 -36.49333 galactic Ari Second-epoch detections are separated by 1.7" and 9.3 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 | 02:33:16.64 +20:21:30.8 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.313+/-0.028 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:16.64 +20:21:30.8: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:16.64 +20:21:30.8: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 33 16.64 +20 21 30.8 11.9 U Ari 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,2461231.8767,11.95,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.48 02:27:17.40 +17:58:32.1
152.86259 -39.26133 galactic Ari Second-epoch detections are separated by 0.4" and 9.6 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 85690060753602944 | 02:27:17.36 +17:58:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.934+/-0.027 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:17.40 +17:58:32.1: 12.64 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:17.40 +17:58:32.1: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 27 17.40 +17 58 32.1 11.5 U Ari 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 85690060753602944,2461231.8767,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 85690060753602944 20260710.3767 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.71 02:29:19.15 +18:04:19.3
153.35269 -38.94929 galactic Ari Second-epoch detections are separated by 1.0" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 85739263898954112 | 02:29:19.16 +18:04:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.396+/-0.030 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:19.15 +18:04:19.3: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:19.15 +18:04:19.3: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 19.15 +18 04 19.3 11.7 U Ari 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 85739263898954112,2461231.8767,11.71,0.05,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
Gaia DR3 85739263898954112 20260710.3767 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 10.3767 2461231.8767 11.65 02:29:32.89 +18:19:41.3
153.25844 -38.69797 galactic Ari Second-epoch detections are separated by 0.4" and 9.5 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 85817058641924736 | 02:29:32.84 +18:19:41.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G2 (LAMOST DR5) J-Ks=0.480+/-0.030 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:32.89 +18:19:41.3: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:32.89 +18:19:41.3: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 32.89 +18 19 41.3 11.7 U Ari 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
Large-amplitude variable Gaia DR2 85817058641924736,2461231.8767,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 85817058641924736 20260710.3767 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.07 02:54:35.44 +21:57:40.9
157.22362 -32.58495 galactic Ari Second-epoch detections are separated by 0.9" and 9.2 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 | 02:54:35.44 +21:57:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:35.44 +21:57:40.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:35.44 +21:57:40.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 10.3767* 02 54 35.44 +21 57 40.9 12.1 U Ari 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,2461231.8767,12.07,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.68 02:53:58.97 +21:58:59.1
157.06886 -32.64270 galactic Ari Second-epoch detections are separated by 1.1" and 9.4 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 109540258962247936 | 02:53:58.89 +21:58:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=1.030+/-0.032 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:58.97 +21:58:59.1: 12.72 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:58.97 +21:58:59.1: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 10.3767* 02 53 58.97 +21 58 59.1 11.7 U Ari 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 109540258962247936,2461231.8767,11.68,0.05,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
Gaia DR3 109540258962247936 20260710.3767 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 10.3767 2461231.8767 11.78 02:30:18.69 +20:52:04.5
151.96067 -36.36900 galactic Ari Second-epoch detections are separated by 2.0" and 9.3 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 87464500722142592 | 02:30:18.70 +20:52:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.703+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:18.69 +20:52:04.5: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:18.69 +20:52:04.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 18.69 +20 52 04.5 11.8 U Ari 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 87464500722142592,2461231.8767,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 87464500722142592 20260710.3767 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.79 03:01:56.83 +23:38:27.8
157.80661 -30.25086 galactic Ari Second-epoch detections are separated by 1.6" and 9.3 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 | 03:01:56.83 +23:38:27.8 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.032 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:01:56.83 +23:38:27.8: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:01:56.83 +23:38:27.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 01 56.83 +23 38 27.8 11.8 U Ari 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,2461231.8767,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.80 03:02:43.08 +25:02:52.9
157.07910 -28.98184 galactic Ari Second-epoch detections are separated by 2.0" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 111878851475043456 | 03:02:43.13 +25:02:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.564+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:43.08 +25:02:52.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:43.08 +25:02:52.9: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 02 43.08 +25 02 52.9 11.8 U Ari 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 111878851475043456,2461231.8767,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 111878851475043456 20260710.3767 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.80 02:27:10.58 +18:39:04.0
152.42814 -38.67570 galactic Ari Second-epoch detections are separated by 0.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.7913+18.6516 | 02:27:10.58 +18:39:04.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:10.58 +18:39:04.0: 13.13 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:10.58 +18:39:04.0: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 27 10.58 +18 39 04.0 11.8 U Ari 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 J036.7913+18.6516,2461231.8767,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.7913+18.6516 20260710.3767 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.41 02:29:29.77 +18:16:03.7
153.28119 -38.75705 galactic Ari Second-epoch detections are separated by 0.4" and 9.5 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 85768400957097856 | 02:29:29.78 +18:16:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.028 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:29.77 +18:16:03.7: 12.33 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:29.77 +18:16:03.7: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 10.3767* 02 29 29.77 +18 16 03.7 11.4 U Ari 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 85768400957097856,2461231.8767,11.41,0.05,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 85768400957097856 20260710.3767 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 10.3767 2461231.8767 11.43 02:30:09.00 +19:35:17.0
152.66390 -37.51949 galactic Ari Second-epoch detections are separated by 1.7" and 9.4 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 86478999002076416 | 02:30:09.02 +19:35:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.037 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:09.00 +19:35:17.0: 12.35 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:09.00 +19:35:17.0: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 09.00 +19 35 17.0 11.4 U Ari 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 86478999002076416,2461231.8767,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86478999002076416 20260710.3767 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.91 02:52:53.95 +21:07:47.7
157.36440 -33.49713 galactic Ari Second-epoch detections are separated by 0.5" and 9.3 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 | 02:52:53.95 +21:07:47.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:53.95 +21:07:47.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:53.95 +21:07:47.7: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 52 53.95 +21 07 47.7 11.9 U Ari 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,2461231.8767,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.44 02:28:32.10 +19:13:01.7
152.45665 -38.02523 galactic Ari Second-epoch detections are separated by 1.5" and 9.6 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 86437664236658432 | 02:28:32.09 +19:13:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:32.10 +19:13:01.7: 12.40 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:32.10 +19:13:01.7: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 10.3767* 02 28 32.10 +19 13 01.7 11.4 U Ari 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 86437664236658432,2461231.8767,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86437664236658432 20260710.3767 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.93 02:56:01.46 +22:19:39.0
157.31894 -32.09732 galactic Ari Second-epoch detections are separated by 1.8" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 109481709967944960 | 02:56:01.43 +22:19:40.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:01.46 +22:19:39.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:01.46 +22:19:39.0: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 01.46 +22 19 39.0 11.9 U Ari 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 109481709967944960,2461231.8767,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109481709967944960 20260710.3767 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.16 02:46:40.96 +19:00:22.4
157.24630 -36.07225 galactic Ari Second-epoch detections are separated by 1.6" and 9.3 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 | 02:46:40.96 +19:00:22.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:46:40.96 +19:00:22.4: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:46:40.96 +19:00:22.4: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 46 40.96 +19 00 22.4 12.2 U Ari 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,2461231.8767,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.70 02:29:42.46 +19:09:36.5
152.80107 -37.94637 galactic Ari Second-epoch detections are separated by 1.1" and 9.3 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 86426737839856128 | 02:29:42.43 +19:09:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.748+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:42.46 +19:09:36.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:42.46 +19:09:36.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 42.46 +19 09 36.5 11.7 U Ari 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 86426737839856128,2461231.8767,11.70,0.05,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
Gaia DR3 86426737839856128 20260710.3767 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 10.3767 2461231.8767 12.06 02:57:06.80 +23:28:44.5
156.83343 -30.99381 galactic Ari Second-epoch detections are separated by 1.4" and 9.3 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 | 02:57:06.80 +23:28:44.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.709+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:06.80 +23:28:44.5: 13.23 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:06.80 +23:28:44.5: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 57 06.80 +23 28 44.5 12.1 U Ari 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,2461231.8767,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 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 10.3767 2461231.8767 12.05 02:52:27.12 +20:26:14.0
157.70931 -34.13638 galactic Ari Second-epoch detections are separated by 0.9" and 9.3 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 | 02:52:27.12 +20:26:14.0 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.611+/-0.031 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:27.12 +20:26:14.0: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:27.12 +20:26:14.0: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 52 27.12 +20 26 14.0 12.1 U Ari 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,2461231.8767,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.90 02:59:34.37 +23:23:01.8
157.44494 -30.76596 galactic Ari Second-epoch detections are separated by 1.9" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:59:34.37 +23:23:01.8 (user input) | T | P | (position from user input) J-Ks=0.788+/-0.026 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:59:34.37 +23:23:01.8: 12.99 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:59:34.37 +23:23:01.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 59 34.37 +23 23 01.8 11.9 U Ari 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,2461231.8767,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.95 02:51:04.00 +21:46:00.8
156.52531 -33.18700 galactic Ari Second-epoch detections are separated by 0.5" and 9.4 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 | 02:51:04.00 +21:46:00.8 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:04.00 +21:46:00.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:04.00 +21:46:00.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 51 04.00 +21 46 00.8 11.9 U Ari 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,2461231.8767,11.95,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.66 02:31:36.12 +18:58:03.3
153.41647 -37.90412 galactic Ari Second-epoch detections are separated by 2.2" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 86241538850177152 | 02:31:36.11 +18:58:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.608+/-0.029 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:36.12 +18:58:03.3: 12.57 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:36.12 +18:58:03.3: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 36.12 +18 58 03.3 11.7 U Ari 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 86241538850177152,2461231.8767,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86241538850177152 20260710.3767 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.02 02:29:46.21 +18:33:54.1
153.17441 -38.46436 galactic Ari Second-epoch detections are separated by 1.8" and 9.7 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 | 02:29:46.21 +18:33:54.1 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.609+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:46.21 +18:33:54.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:46.21 +18:33:54.1: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 46.21 +18 33 54.1 12.0 U Ari 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,2461231.8767,12.02,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.56 02:28:14.10 +18:32:32.1
152.77739 -38.65548 galactic Ari Second-epoch detections are separated by 1.0" and 9.4 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 85837674485187840 | 02:28:14.08 +18:32:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.440+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:14.10 +18:32:32.1: 12.59 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:14.10 +18:32:32.1: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 10.3767* 02 28 14.10 +18 32 32.1 11.6 U Ari 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 85837674485187840,2461231.8767,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 85837674485187840 20260710.3767 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.62 02:28:52.26 +17:59:57.8
153.27618 -39.06370 galactic Ari Second-epoch detections are separated by 2.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 85737137890785664 | 02:28:52.24 +17:59:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.374+/-0.025 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:52.26 +17:59:57.8: 12.58 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:52.26 +17:59:57.8: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 10.3767* 02 28 52.26 +17 59 57.8 11.6 U Ari 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 85737137890785664,2461231.8767,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 85737137890785664 20260710.3767 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.07 02:28:24.87 +18:57:20.1
152.57924 -38.27002 galactic Ari Second-epoch detections are separated by 0.6" and 9.6 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 86043042641451264 | 02:28:24.88 +18:57:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.624+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:24.87 +18:57:20.1: 12.02 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:24.87 +18:57:20.1: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 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 10.3767* 02 28 24.87 +18 57 20.1 11.1 U Ari 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 86043042641451264,2461231.8767,11.07,0.05,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
Gaia DR3 86043042641451264 20260710.3767 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.07 02:57:37.01 +22:52:55.8
157.32627 -31.43196 galactic Ari Second-epoch detections are separated by 2.2" and 8.8 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 | 02:57:37.01 +22:52:55.8 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.764+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:37.01 +22:52:55.8: 13.29 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:37.01 +22:52:55.8: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 57 37.01 +22 52 55.8 12.1 U Ari 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,2461231.8767,12.07,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.65 02:50:36.37 +21:14:36.0
156.74958 -33.68756 galactic Ari Second-epoch detections are separated by 1.0" and 9.3 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 85466069619473152 | 02:50:36.33 +21:14:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.348+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:36.37 +21:14:36.0: 12.57 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:36.37 +21:14:36.0: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 50 36.37 +21 14 36.0 11.7 U Ari 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 85466069619473152,2461231.8767,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 85466069619473152 20260710.3767 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.05 02:56:17.79 +22:24:50.6
157.32573 -31.99047 galactic Ari Second-epoch detections are separated by 2.0" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:56:17.79 +22:24:50.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.887+/-0.028 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:17.79 +22:24:50.6: 13.29 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:17.79 +22:24:50.6: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 17.79 +22 24 50.6 12.1 U Ari 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,2461231.8767,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.88 02:30:08.49 +19:34:38.8
152.66793 -37.52981 galactic Ari Second-epoch detections are separated by 0.7" and 9.4 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 86478999002076416 | 02:30:09.02 +19:35:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.385+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:08.49 +19:34:38.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:08.49 +19:34:38.8: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 08.49 +19 34 38.8 11.9 U Ari 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 86478999002076416,2461231.8767,11.88,0.05,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
Gaia DR3 86478999002076416 20260710.3767 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 10.3767 2461231.8767 11.71 02:28:08.42 +17:47:32.8
153.20446 -39.32819 galactic Ari Second-epoch detections are separated by 2.1" and 9.5 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 | 02:28:08.42 +17:47:32.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.434+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:08.42 +17:47:32.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:08.42 +17:47:32.8: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 08.42 +17 47 32.8 11.7 U Ari 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,2461231.8767,11.71,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.73 02:27:25.21 +18:05:46.8
152.82518 -39.14010 galactic Ari Second-epoch detections are separated by 1.3" and 9.7 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 | 02:27:25.21 +18:05:46.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.475+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:25.21 +18:05:46.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:25.21 +18:05:46.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 27 25.21 +18 05 46.8 11.7 U Ari 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,2461231.8767,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.96 02:49:40.89 +20:51:37.7
156.77422 -34.12654 galactic Ari Second-epoch detections are separated by 1.3" and 9.5 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 | 02:49:40.89 +20:51:37.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.763+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:40.89 +20:51:37.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:40.89 +20:51:37.7: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 49 40.89 +20 51 37.7 12.0 U Ari 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,2461231.8767,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.02 02:48:45.83 +20:45:32.2
156.61911 -34.32617 galactic Ari Second-epoch detections are separated by 2.4" and 9.6 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 | 02:48:45.83 +20:45:32.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.365+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:48:45.83 +20:45:32.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:48:45.83 +20:45:32.2: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 48 45.83 +20 45 32.2 12.0 U Ari 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,2461231.8767,12.02,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.91 02:57:12.48 +23:33:18.8
156.80663 -30.91800 galactic Ari Second-epoch detections are separated by 0.6" and 9.3 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 | 02:57:12.48 +23:33:18.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.821+/-0.027 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:12.48 +23:33:18.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:12.48 +23:33:18.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 57 12.48 +23 33 18.8 11.9 U Ari 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,2461231.8767,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.60 03:02:00.60 +23:46:00.2
157.73971 -30.13836 galactic Ari Second-epoch detections are separated by 0.2" and 9.2 pix
The object was found in VSX 0" NSVS 6623348
Type: EB
# Max. Min./Amp. JD0 Period
12.410 R1 Y 0.490 R1 4.155279600000
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:00.60 +23:46:00.2: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:00.60 +23:46:00.2: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 10.3767* 03 02 00.60 +23 46 00.2 11.6 U Ari 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
NSVS 6623348,2461231.8767,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6623348 20260710.3767 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.61 02:53:35.23 +22:27:31.7
156.67463 -32.29047 galactic Ari Second-epoch detections are separated by 1.0" and 9.4 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 109660616830022016 | 02:53:35.22 +22:27:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.703+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:35.23 +22:27:31.7: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:35.23 +22:27:31.7: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 10.3767* 02 53 35.23 +22 27 31.7 11.6 U Ari 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 109660616830022016,2461231.8767,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109660616830022016 20260710.3767 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.49 02:30:49.45 +19:31:49.0
152.87484 -37.49586 galactic Ari Second-epoch detections are separated by 1.1" and 9.4 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 86463292306426624 | 02:30:49.49 +19:31:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.149+/-0.029 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:49.45 +19:31:49.0: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:49.45 +19:31:49.0: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 49.45 +19 31 49.0 11.5 U Ari 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 86463292306426624,2461231.8767,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86463292306426624 20260710.3767 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.40 02:27:59.79 +18:29:42.7
152.74148 -38.72349 galactic Ari Second-epoch detections are separated by 1.2" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 85837086074079360 | 02:27:59.75 +18:29:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.701+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:59.79 +18:29:42.7: 12.54 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:59.79 +18:29:42.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 10.3767* 02 27 59.79 +18 29 42.7 11.4 U Ari 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 85837086074079360,2461231.8767,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 85837086074079360 20260710.3767 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.64 02:54:48.92 +23:33:35.0
156.26396 -31.20883 galactic Ari Second-epoch detections are separated by 0.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1433 Geramtina -42 227 231 16.9 0 0
ATTENTION: measured mag 11.64 is 5.3 mag brighter than the predicted asteroid brightness 16.9 - the transient may be an unrelated new object!
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:48.92 +23:33:35.0: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:48.92 +23:33:35.0: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 10.3767* 02 54 48.92 +23 33 35.0 11.6 U Ari 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,2461231.8767,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3767 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.57 02:53:16.08 +23:07:39.0
156.18099 -31.76377 galactic Ari Second-epoch detections are separated by 0.7" and 9.1 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 112768596900132864 | 02:53:16.03 +23:07:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.125+/-0.036 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:16.08 +23:07:39.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:16.08 +23:07:39.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 10.3767* 02 53 16.08 +23 07 39.0 11.6 U Ari 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 112768596900132864,2461231.8767,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 112768596900132864 20260710.3767 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.82 02:27:13.03 +18:34:05.4
152.48832 -38.74475 galactic Ari Second-epoch detections are separated by 0.4" and 9.5 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 | 02:27:13.03 +18:34:05.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.658+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:13.03 +18:34:05.4: 13.23 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:13.03 +18:34:05.4: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 27 13.03 +18 34 05.4 11.8 U Ari 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,2461231.8767,11.82,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.89 02:29:13.86 +19:27:59.3
152.49387 -37.72814 galactic Ari Second-epoch detections are separated by 2.9" and 9.4 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 | 02:29:13.86 +19:27:59.3 (user input) | T | P | (position from user input) J-Ks=0.625+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:13.86 +19:27:59.3: 13.24 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:13.86 +19:27:59.3: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 13.86 +19 27 59.3 11.9 U Ari 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,2461231.8767,11.89,0.05,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 20260710.3767 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 10.3767 2461231.8767 12.02 02:51:12.57 +21:49:55.4
156.51761 -33.11417 galactic Ari Second-epoch detections are separated by 0.8" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:51:12.57 +21:49:55.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.805+/-0.029 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:12.57 +21:49:55.4: 13.22 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:12.57 +21:49:55.4: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 51 12.57 +21 49 55.4 12.0 U Ari 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,2461231.8767,12.02,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.80 02:55:06.42 +22:49:48.3
156.78879 -31.78902 galactic Ari Second-epoch detections are separated by 0.1" and 9.2 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 | 02:55:06.42 +22:49:48.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.733+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:06.42 +22:49:48.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:06.42 +22:49:48.3: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 55 06.42 +22 49 48.3 11.8 U Ari 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,2461231.8767,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.04 02:48:36.57 +19:31:40.9
157.37827 -35.38845 galactic Ari Second-epoch detections are separated by 1.1" and 9.4 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 | 02:48:36.57 +19:31:40.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.416+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:48:36.57 +19:31:40.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:48:36.57 +19:31:40.9: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 48 36.57 +19 31 40.9 12.0 U Ari 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,2461231.8767,12.04,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.94 02:54:30.94 +23:08:45.4
156.45472 -31.59540 galactic Ari Second-epoch detections are separated by 1.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:54:30.94 +23:08:45.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.457+/-0.034 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:30.94 +23:08:45.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:30.94 +23:08:45.4: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 54 30.94 +23 08 45.4 11.9 U Ari 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,2461231.8767,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.96 02:55:34.49 +22:04:48.9
157.37448 -32.36142 galactic Ari Second-epoch detections are separated by 0.9" and 9.4 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 | 02:55:34.49 +22:04:48.9 (user input) | T | P | (position from user input) J-Ks=0.725+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:34.49 +22:04:48.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:34.49 +22:04:48.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 55 34.49 +22 04 48.9 12.0 U Ari 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,2461231.8767,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 10.93 02:28:33.47 +18:46:22.6
152.72607 -38.41578 galactic Ari Second-epoch detections are separated by 0.3" and 9.5 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 86035552218493312 | 02:28:33.43 +18:46:22.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.890+/-0.028 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:33.47 +18:46:22.6: 11.84 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:33.47 +18:46:22.6: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 33.47 +18 46 22.6 10.9 U Ari 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 86035552218493312,2461231.8767,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86035552218493312 20260710.3767 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.72 02:30:28.63 +19:37:44.4
152.72545 -37.44719 galactic Ari Second-epoch detections are separated by 1.9" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:30:28.63 +19:37:44.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.404+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:28.63 +19:37:44.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:28.63 +19:37:44.4: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 28.63 +19 37 44.4 11.7 U Ari 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,2461231.8767,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.88 02:33:02.59 +21:37:56.6
152.21705 -35.39619 galactic Ari Second-epoch detections are separated by 2.1" and 9.3 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 | 02:33:02.59 +21:37:56.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.413+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:02.59 +21:37:56.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:02.59 +21:37:56.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 33 02.59 +21 37 56.6 11.9 U Ari 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,2461231.8767,11.88,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.94 02:49:52.83 +20:58:13.7
156.75133 -34.00864 galactic Ari Second-epoch detections are separated by 0.3" and 9.4 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 85250913233015680 | 02:49:52.80 +20:58:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.704+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:52.83 +20:58:13.7: 12.91 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:52.83 +20:58:13.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 49 52.83 +20 58 13.7 11.9 U Ari 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 85250913233015680,2461231.8767,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 85250913233015680 20260710.3767 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.79 02:28:30.72 +18:15:36.8
153.02131 -38.87385 galactic Ari Second-epoch detections are separated by 1.5" and 9.6 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 | 02:28:30.72 +18:15:36.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.478+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:30.72 +18:15:36.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:30.72 +18:15:36.8: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 30.72 +18 15 36.8 11.8 U Ari 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,2461231.8767,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.88 02:31:48.31 +20:53:33.4
152.32960 -36.18494 galactic Ari Second-epoch detections are separated by 1.5" and 9.8 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 | 02:31:48.31 +20:53:33.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.673+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:48.31 +20:53:33.4: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:48.31 +20:53:33.4: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 48.31 +20 53 33.4 11.9 U Ari 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,2461231.8767,11.88,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.79 02:28:31.84 +19:33:46.3
152.25250 -37.71935 galactic Ari Second-epoch detections are separated by 0.3" and 9.5 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 | 02:28:31.84 +19:33:46.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:31.84 +19:33:46.3: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:31.84 +19:33:46.3: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 31.84 +19 33 46.3 11.8 U Ari 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,2461231.8767,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.58 02:30:21.31 +20:14:14.3
152.33660 -36.92290 galactic Ari Second-epoch detections are separated by 0.8" and 9.5 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 86652339586579840 | 02:30:21.31 +20:14:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:21.31 +20:14:14.3: 12.50 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:21.31 +20:14:14.3: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 10.3767* 02 30 21.31 +20 14 14.3 11.6 U Ari 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 86652339586579840,2461231.8767,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86652339586579840 20260710.3767 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.03 02:53:40.58 +22:49:15.5
156.46671 -31.97332 galactic Ari Second-epoch detections are separated by 0.6" and 9.2 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 | 02:53:40.58 +22:49:15.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.880+/-0.034 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:40.58 +22:49:15.5: 13.21 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:40.58 +22:49:15.5: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 10.3767* 02 53 40.58 +22 49 15.5 12.0 U Ari 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,2461231.8767,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.03 02:52:15.94 +21:57:30.0
156.68493 -32.87695 galactic Ari Second-epoch detections are separated by 2.8" and 9.6 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 | 02:52:15.94 +21:57:30.0 (user input) | T | P | (position from user input) J-Ks=0.849+/-0.032 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:15.94 +21:57:30.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:15.94 +21:57:30.0: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 52 15.94 +21 57 30.0 12.0 U Ari 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,2461231.8767,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.00 02:59:38.51 +23:05:13.2
157.65066 -31.00510 galactic Ari Second-epoch detections are separated by 0.7" and 9.1 pix
The object was found in VSX 2" Gaia DR3 109911584654704640
Type: RS
# Max. Min./Amp. JD0 Period
12.820 G 12.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:59:38.51 +23:05:13.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:59:38.51 +23:05:13.2: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 59 38.51 +23 05 13.2 12.0 U Ari 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 109911584654704640,2461231.8767,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109911584654704640 20260710.3767 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.57 02:56:19.34 +23:20:15.6
156.74429 -31.21082 galactic Ari Second-epoch detections are separated by 0.7" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J044.0804+23.3377 | 02:56:19.30 +23:20:15.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.705+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:19.34 +23:20:15.6: 12.47 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:19.34 +23:20:15.6: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 19.34 +23 20 15.6 11.6 U Ari 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 J044.0804+23.3377,2461231.8767,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J044.0804+23.3377 20260710.3767 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.51 02:30:08.58 +20:04:49.8
152.37288 -37.08485 galactic Ari Second-epoch detections are separated by 1.7" and 9.4 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 J037.5357+20.0805 | 02:30:08.57 +20:04:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:08.58 +20:04:49.8: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:08.58 +20:04:49.8: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 08.58 +20 04 49.8 11.5 U Ari 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 J037.5357+20.0805,2461231.8767,11.51,0.05,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
ATO J037.5357+20.0805 20260710.3767 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 10.3767 2461231.8767 11.45 02:29:14.53 +19:32:29.3
152.45269 -37.66054 galactic Ari Second-epoch detections are separated by 0.9" and 9.4 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 86519023801472384 | 02:29:14.32 +19:32:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2.5e 2013AJ....145..102L PM J02292+1932
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:14.53 +19:32:29.3: 12.44 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:14.53 +19:32:29.3: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 14.53 +19 32 29.3 11.4 U Ari 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 86519023801472384,2461231.8767,11.45,0.05,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 86519023801472384 20260710.3767 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 10.3767 2461231.8767 11.40 02:29:42.97 +18:46:27.0
153.03407 -38.28604 galactic Ari Second-epoch detections are separated by 0.5" and 9.5 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 | 02:29:42.97 +18:46:27.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.421+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:42.97 +18:46:27.0: 12.43 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:42.97 +18:46:27.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 42.97 +18 46 27.0 11.4 U Ari 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,2461231.8767,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.51 02:30:21.06 +18:44:38.5
153.22087 -38.24156 galactic Ari Second-epoch detections are separated by 1.3" and 9.3 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 86209442559103872 | 02:30:21.02 +18:44:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.316+/-0.029 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:21.06 +18:44:38.5: 12.41 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:21.06 +18:44:38.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 30 21.06 +18 44 38.5 11.5 U Ari 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 86209442559103872,2461231.8767,11.51,0.05,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 86209442559103872 20260710.3767 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 10.3767 2461231.8767 11.95 02:56:09.44 +22:24:59.0
157.29241 -32.00599 galactic Ari Second-epoch detections are separated by 1.7" and 9.5 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 | 02:56:09.44 +22:24:59.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.821+/-0.028 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:09.44 +22:24:59.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:09.44 +22:24:59.0: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 09.44 +22 24 59.0 11.9 U Ari 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,2461231.8767,11.95,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.98 02:31:15.18 +19:53:45.4
152.77017 -37.12577 galactic Ari Second-epoch detections are separated by 1.7" and 9.6 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 | 02:31:15.18 +19:53:45.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:15.18 +19:53:45.4: 13.17 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:15.18 +19:53:45.4: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 15.18 +19 53 45.4 12.0 U Ari 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,2461231.8767,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.82 02:29:41.93 +20:05:42.6
152.24856 -37.12034 galactic Ari Second-epoch detections are separated by 1.0" and 9.7 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 | 02:29:41.93 +20:05:42.6 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.389+/-0.026 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:41.93 +20:05:42.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:41.93 +20:05:42.6: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 41.93 +20 05 42.6 11.8 U Ari 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,2461231.8767,11.82,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.96 02:51:56.11 +20:24:47.8
157.60187 -34.22202 galactic Ari Second-epoch detections are separated by 1.6" and 9.4 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 | 02:51:56.11 +20:24:47.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.417+/-0.036 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:56.11 +20:24:47.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:56.11 +20:24:47.8: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 51 56.11 +20 24 47.8 12.0 U Ari 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,2461231.8767,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.30 02:27:25.58 +18:07:17.2
152.81174 -39.11721 galactic Ari Second-epoch detections are separated by 1.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8560+18.1215 | 02:27:25.46 +18:07:17.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:25.58 +18:07:17.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:25.58 +18:07:17.2: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 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 10.3767* 02 27 25.58 +18 07 17.2 11.3 U Ari 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 J036.8560+18.1215,2461231.8767,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.8560+18.1215 20260710.3767 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.29 02:48:43.22 +20:12:41.1
156.96054 -34.79610 galactic Ari Second-epoch detections are separated by 0.7" and 9.3 pix
The object was found in VSX 0" ASAS J024843+2012.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.300 V Y 0.410 V 2452871.20000 198.142000000000
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:48:43.22 +20:12:41.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:48:43.22 +20:12:41.1: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 10.3767* 02 48 43.22 +20 12 41.1 11.3 U Ari 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
ASAS J024843+2012.6,2461231.8767,11.29,0.05,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
ASAS J024843+2012.6 20260710.3767 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 10.3767 2461231.8767 11.89 02:28:28.65 +18:56:39.4
152.60274 -38.27309 galactic Ari Second-epoch detections are separated by 0.9" and 9.4 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 | 02:28:28.65 +18:56:39.4 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:28.65 +18:56:39.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:28.65 +18:56:39.4: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 28.65 +18 56 39.4 11.9 U Ari 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,2461231.8767,11.89,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.86 02:27:24.52 +18:15:11.2
152.72793 -39.00267 galactic Ari Second-epoch detections are separated by 0.9" and 9.6 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 | 02:27:24.52 +18:15:11.2 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:24.52 +18:15:11.2: 13.13 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:24.52 +18:15:11.2: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 27 24.52 +18 15 11.2 11.9 U Ari 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,2461231.8767,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.86 02:53:05.73 +22:57:22.4
156.24841 -31.93000 galactic Ari Second-epoch detections are separated by 0.2" and 9.3 pix
The object was found in VSX 4" Gaia DR3 109739682883625728
Type: ROT
# Max. Min./Amp. JD0 Period
12.430 G 12.460 G
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:05.73 +22:57:22.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:05.73 +22:57:22.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 53 05.73 +22 57 22.4 11.9 U Ari 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 109739682883625728,2461231.8767,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109739682883625728 20260710.3767 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.85 03:03:41.47 +24:55:39.4
157.36522 -28.96016 galactic Ari Second-epoch detections are separated by 2.9" and 8.7 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 | 03:03:41.47 +24:55:39.4 (user input) | T | P | (position from user input) J-Ks=0.602+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:03:41.47 +24:55:39.4: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:03:41.47 +24:55:39.4: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 10.3767* 03 03 41.47 +24 55 39.4 11.8 U Ari 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,2461231.8767,11.85,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.88 02:50:21.82 +22:30:29.6
155.89496 -32.64288 galactic Ari Second-epoch detections are separated by 0.8" and 9.4 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 | 02:50:21.82 +22:30:29.6 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:21.82 +22:30:29.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:21.82 +22:30:29.6: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 50 21.82 +22 30 29.6 11.9 U Ari 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,2461231.8767,11.88,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.80 02:32:22.04 +18:29:35.3
153.90776 -38.23327 galactic Ari Second-epoch detections are separated by 2.5" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:22.04 +18:29:35.3 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.371+/-0.027 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:32:22.04 +18:29:35.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:32:22.04 +18:29:35.3: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 32 22.04 +18 29 35.3 11.8 U Ari 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,2461231.8767,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.96 02:28:50.02 +19:14:10.1
152.52464 -37.97562 galactic Ari Second-epoch detections are separated by 0.6" and 9.6 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 | 02:28:50.02 +19:14:10.1 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.644+/-0.029 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:50.02 +19:14:10.1: 13.13 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:50.02 +19:14:10.1: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 50.02 +19 14 10.1 12.0 U Ari 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,2461231.8767,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.88 02:56:19.03 +23:32:13.3
156.61762 -31.04352 galactic Ari Second-epoch detections are separated by 2.2" and 9.2 pix
The object was found in VSX 1" Gaia DR3 110180965003517952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.690 G 12.710 G F
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:19.03 +23:32:13.3: 12.83 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:19.03 +23:32:13.3: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 19.03 +23 32 13.3 11.9 U Ari 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 110180965003517952,2461231.8767,11.88,0.05,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
Gaia DR3 110180965003517952 20260710.3767 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 10.3767 2461231.8767 11.87 02:50:18.15 +21:55:47.4
156.24261 -33.14240 galactic Ari Second-epoch detections are separated by 0.6" and 9.4 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 109571354525411072 | 02:50:18.16 +21:55:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.702+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:18.15 +21:55:47.4: 12.82 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:18.15 +21:55:47.4: 12.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 50 18.15 +21 55 47.4 11.9 U Ari 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 109571354525411072,2461231.8767,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109571354525411072 20260710.3767 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.85 03:00:42.75 +23:23:52.6
157.68963 -30.61007 galactic Ari Second-epoch detections are separated by 1.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:00:42.75 +23:23:52.6 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.033 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:42.75 +23:23:52.6: 12.82 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:42.75 +23:23:52.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 00 42.75 +23 23 52.6 11.8 U Ari 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,2461231.8767,11.85,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.87 02:55:42.50 +22:27:25.2
157.16363 -32.02817 galactic Ari Second-epoch detections are separated by 1.4" and 9.4 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 | 02:55:42.50 +22:27:25.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.395+/-0.027 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:42.50 +22:27:25.2: 12.82 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:42.50 +22:27:25.2: 12.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 55 42.50 +22 27 25.2 11.9 U Ari 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,2461231.8767,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.72 02:29:46.13 +20:07:50.1
152.24620 -37.08135 galactic Ari Second-epoch detections are separated by 2.1" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:29:46.13 +20:07:50.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.343+/-0.031 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:46.13 +20:07:50.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:46.13 +20:07:50.1: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 46.13 +20 07 50.1 11.7 U Ari 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,2461231.8767,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.83 02:29:02.28 +20:00:35.7
152.12543 -37.26776 galactic Ari Second-epoch detections are separated by 2.2" and 9.7 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 | 02:29:02.28 +20:00:35.7 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.332+/-0.025 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:02.28 +20:00:35.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:02.28 +20:00:35.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 02.28 +20 00 35.7 11.8 U Ari 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,2461231.8767,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.79 02:31:20.06 +18:40:07.5
153.52712 -38.19691 galactic Ari Second-epoch detections are separated by 0.7" and 9.5 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 | 02:31:20.06 +18:40:07.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.455+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:20.06 +18:40:07.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:20.06 +18:40:07.5: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 10.3767* 02 31 20.06 +18 40 07.5 11.8 U Ari 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,2461231.8767,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.82 02:52:18.73 +22:57:00.0
156.07196 -32.03078 galactic Ari Second-epoch detections are separated by 0.8" and 9.2 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 112741379691536128 | 02:52:18.73 +22:56:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.030 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:18.73 +22:57:00.0: 12.78 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:18.73 +22:57:00.0: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 10.3767* 02 52 18.73 +22 57 00.0 11.8 U Ari 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 112741379691536128,2461231.8767,11.82,0.05,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
Gaia DR3 112741379691536128 20260710.3767 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 10.3767 2461231.8767 11.81 02:56:37.30 +23:21:34.6
156.79805 -31.15526 galactic Ari Second-epoch detections are separated by 1.0" and 9.1 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 110142649599806976 | 02:56:37.27 +23:21:34.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.729+/-0.026 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:37.30 +23:21:34.6: 12.80 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:37.30 +23:21:34.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 37.30 +23 21 34.6 11.8 U Ari 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 110142649599806976,2461231.8767,11.81,0.05,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
Gaia DR3 110142649599806976 20260710.3767 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 10.3767 2461231.8767 11.80 03:05:01.43 +24:56:46.5
157.63989 -28.77643 galactic Ari Second-epoch detections are separated by 1.1" and 9.2 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 | 03:05:01.43 +24:56:46.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.460+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:05:01.43 +24:56:46.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:05:01.43 +24:56:46.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 05 01.43 +24 56 46.5 11.8 U Ari 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,2461231.8767,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.81 03:04:13.32 +24:22:02.2
157.83733 -29.35834 galactic Ari Second-epoch detections are separated by 1.0" and 9.3 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 111781265522296960 | 03:04:13.26 +24:22:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.026 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:13.32 +24:22:02.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:13.32 +24:22:02.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 04 13.32 +24 22 02.2 11.8 U Ari 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 111781265522296960,2461231.8767,11.81,0.05,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
Gaia DR3 111781265522296960 20260710.3767 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 10.3767 2461231.8767 11.82 02:29:46.30 +20:01:14.7
152.31092 -37.17831 galactic Ari Second-epoch detections are separated by 1.7" and 9.7 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 | 02:29:46.30 +20:01:14.7 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.027 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:46.30 +20:01:14.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:46.30 +20:01:14.7: 12.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 46.30 +20 01 14.7 11.8 U Ari 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,2461231.8767,11.82,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.79 02:31:53.76 +18:26:16.9
153.81688 -38.33545 galactic Ari Second-epoch detections are separated by 2.0" and 9.8 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 | 02:31:53.76 +18:26:16.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.372+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:53.76 +18:26:16.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:53.76 +18:26:16.9: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 53.76 +18 26 16.9 11.8 U Ari 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,2461231.8767,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.90 02:31:16.30 +19:55:45.8
152.75527 -37.09420 galactic Ari Second-epoch detections are separated by 1.6" and 9.2 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 | 02:31:16.30 +19:55:45.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.432+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:16.30 +19:55:45.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:16.30 +19:55:45.8: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 16.30 +19 55 45.8 11.9 U Ari 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,2461231.8767,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.77 02:58:18.32 +22:31:40.7
157.70974 -31.64137 galactic Ari Second-epoch detections are separated by 3.5" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 109851691335029376 | 02:58:18.28 +22:31:40.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.439+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:58:18.32 +22:31:40.7: 12.76 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:58:18.32 +22:31:40.7: 12.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 58 18.32 +22 31 40.7 11.8 U Ari 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 109851691335029376,2461231.8767,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109851691335029376 20260710.3767 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.86 02:31:26.15 +19:16:05.3
153.19169 -37.65854 galactic Ari Second-epoch detections are separated by 0.2" and 9.4 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 | 02:31:26.15 +19:16:05.3 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.026 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:26.15 +19:16:05.3: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:26.15 +19:16:05.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 26.15 +19 16 05.3 11.9 U Ari 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,2461231.8767,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.81 02:50:01.35 +20:47:09.6
156.90357 -34.14732 galactic Ari Second-epoch detections are separated by 2.5" and 9.6 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 | 02:50:01.35 +20:47:09.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.346+/-0.029 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:01.35 +20:47:09.6: 12.74 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:01.35 +20:47:09.6: 12.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 50 01.35 +20 47 09.6 11.8 U Ari 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,2461231.8767,11.81,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.71 03:04:46.11 +25:12:30.3
157.41846 -28.59112 galactic Ari Second-epoch detections are separated by 0.5" and 9.2 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 | 03:04:46.11 +25:12:30.3 (user input) | T | P | (position from user input) J-Ks=0.712+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:46.11 +25:12:30.3: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:46.11 +25:12:30.3: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 04 46.11 +25 12 30.3 11.7 U Ari 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,2461231.8767,11.71,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.81 03:02:49.20 +24:37:31.6
157.36854 -29.32127 galactic Ari Second-epoch detections are separated by 3.2" and 8.9 pix
The object was found in VSX 0" ASASSN-V J030249.17+243731.6
Type: ROT
# Max. Min./Amp. JD0 Period
13.170 g Y 0.090 g 2459487.96800 14.341000000000
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:49.20 +24:37:31.6: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:49.20 +24:37:31.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 02 49.20 +24 37 31.6 11.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J030249.17+243731.6,2461231.8767,11.81,0.05,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
ASASSN-V J030249.17+243731.6 20260710.3767 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 10.3767 2461231.8767 11.89 02:29:01.86 +19:56:30.6
152.16315 -37.32890 galactic Ari Second-epoch detections are separated by 2.7" and 9.8 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 | 02:29:01.86 +19:56:30.6 (user input) | T | P | (position from user input) J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:01.86 +19:56:30.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:01.86 +19:56:30.6: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 10.3767* 02 29 01.86 +19 56 30.6 11.9 U Ari 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,2461231.8767,11.89,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.78 02:30:30.19 +21:14:03.8
151.80022 -36.02326 galactic Ari Second-epoch detections are separated by 1.0" and 9.5 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 89023097109910400 | 02:30:30.13 +21:14:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.477+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:30.19 +21:14:03.8: 12.71 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:30.19 +21:14:03.8: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 10.3767* 02 30 30.19 +21 14 03.8 11.8 U Ari 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 89023097109910400,2461231.8767,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 89023097109910400 20260710.3767 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.74 02:31:01.93 +18:43:33.7
153.41234 -38.18074 galactic Ari Second-epoch detections are separated by 1.4" and 9.6 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 86210851308377216 | 02:31:01.87 +18:43:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.661+/-0.030 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:01.93 +18:43:33.7: 12.71 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:01.93 +18:43:33.7: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 01.93 +18 43 33.7 11.7 U Ari 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 86210851308377216,2461231.8767,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86210851308377216 20260710.3767 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.65 02:49:24.89 +20:11:35.0
157.14038 -34.72498 galactic Ari Second-epoch detections are separated by 2.0" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 85066092199989504 | 02:49:24.92 +20:11:36.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:24.89 +20:11:35.0: 12.70 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:24.89 +20:11:35.0: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 49 24.89 +20 11 35.0 11.7 U Ari 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
Large-amplitude variable Gaia DR2 85066092199989504,2461231.8767,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 85066092199989504 20260710.3767 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.67 03:01:53.91 +24:08:51.3
157.47160 -29.83541 galactic Ari Second-epoch detections are separated by 2.0" and 9.1 pix
The object was found in VSX 4" ASASSN-V J030153.77+240847.8
Type: ROT
# Max. Min./Amp. JD0 Period
13.350 g Y 0.190 g 2458808.66000 5.692000000000
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:01:53.91 +24:08:51.3: 12.74 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:01:53.91 +24:08:51.3: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 01 53.91 +24 08 51.3 11.7 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J030153.77+240847.8,2461231.8767,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J030153.77+240847.8 20260710.3767 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.21 02:28:40.63 +18:49:53.8
152.72296 -38.35072 galactic Ari Second-epoch detections are separated by 0.6" and 9.5 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 86038056183928448 | 02:28:40.60 +18:49:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.485+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:40.63 +18:49:53.8: 12.25 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:40.63 +18:49:53.8: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 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 10.3767* 02 28 40.63 +18 49 53.8 11.2 U Ari 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 86038056183928448,2461231.8767,11.21,0.05,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 86038056183928448 20260710.3767 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 10.3767 2461231.8767 11.23 02:27:13.42 +18:36:47.5
152.46335 -38.70412 galactic Ari Second-epoch detections are separated by 1.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 86006788822020224 | 02:27:13.41 +18:36:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.413+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:13.42 +18:36:47.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:13.42 +18:36:47.5: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 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 10.3767* 02 27 13.42 +18 36 47.5 11.2 U Ari 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 86006788822020224,2461231.8767,11.23,0.05,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 86006788822020224 20260710.3767 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 10.3767 2461231.8767 11.15 02:27:49.85 +18:34:08.4
152.65289 -38.67648 galactic Ari Second-epoch detections are separated by 1.0" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.9576+18.5689 | 02:27:49.82 +18:34:08.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.747+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:49.85 +18:34:08.4: 12.20 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:49.85 +18:34:08.4: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 10.3767* 02 27 49.85 +18 34 08.4 11.2 U Ari 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 J036.9576+18.5689,2461231.8767,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.9576+18.5689 20260710.3767 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.07 02:50:46.33 +20:53:17.1
157.01681 -33.96759 galactic Ari Second-epoch detections are separated by 2.4" and 9.7 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 | 02:50:46.33 +20:53:17.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.626+/-0.026 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:46.33 +20:53:17.1: 13.10 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:46.33 +20:53:17.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 10.3767* 02 50 46.33 +20 53 17.1 12.1 U Ari 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,2461231.8767,12.07,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.67 02:31:17.58 +18:57:25.4
153.34143 -37.94822 galactic Ari Second-epoch detections are separated by 0.5" and 9.5 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 86218925846888192 | 02:31:17.56 +18:57:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.691+/-0.029 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:17.58 +18:57:25.4: 12.70 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:17.58 +18:57:25.4: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 17.58 +18 57 25.4 11.7 U Ari 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 86218925846888192,2461231.8767,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86218925846888192 20260710.3767 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.70 02:31:59.23 +21:20:47.7
152.11415 -35.76364 galactic Ari Second-epoch detections are separated by 1.9" and 9.6 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 88980903351243136 | 02:31:59.13 +21:20:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.461+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:59.23 +21:20:47.7: 12.70 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:59.23 +21:20:47.7: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 31 59.23 +21 20 47.7 11.7 U Ari 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 88980903351243136,2461231.8767,11.70,0.05,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
Gaia DR3 88980903351243136 20260710.3767 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 10.3767 2461231.8767 12.11 02:28:22.95 +19:07:52.9
152.46674 -38.11791 galactic Ari Second-epoch detections are separated by 0.7" and 9.4 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 | 02:28:22.95 +19:07:52.9 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:22.95 +19:07:52.9: 13.61 +/- 0.03 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:22.95 +19:07:52.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 28 22.95 +19 07 52.9 12.1 U Ari 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,2461231.8767,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.77 02:33:19.66 +21:35:48.2
152.30922 -35.39668 galactic Ari Second-epoch detections are separated by 0.7" and 9.4 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 89014709038126720 | 02:33:19.56 +21:35:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.704+/-0.024 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:19.66 +21:35:48.2: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:19.66 +21:35:48.2: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 33 19.66 +21 35 48.2 11.8 U Ari 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 89014709038126720,2461231.8767,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 89014709038126720 20260710.3767 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.72 02:55:07.53 +23:04:39.9
156.63660 -31.57787 galactic Ari Second-epoch detections are separated by 1.2" and 9.2 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 109756347356751360 | 02:55:07.48 +23:04:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.705+/-0.026 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:07.53 +23:04:39.9: 12.68 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:07.53 +23:04:39.9: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 55 07.53 +23 04 39.9 11.7 U Ari 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 109756347356751360,2461231.8767,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 109756347356751360 20260710.3767 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.68 03:04:26.67 +25:44:22.2
157.01410 -28.19006 galactic Ari Second-epoch detections are separated by 2.2" and 9.1 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 115020259275493376 | 03:04:26.71 +25:44:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.425+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:26.67 +25:44:22.2: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:26.67 +25:44:22.2: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 04 26.67 +25 44 22.2 11.7 U Ari 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 115020259275493376,2461231.8767,11.68,0.05,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
Gaia DR3 115020259275493376 20260710.3767 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 10.3767 2461231.8767 11.67 03:04:39.28 +25:05:11.8
157.47141 -28.70663 galactic Ari Second-epoch detections are separated by 2.3" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 111959111528094592 | 03:04:39.17 +25:05:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.445+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:39.28 +25:05:11.8: 12.68 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:39.28 +25:05:11.8: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 04 39.28 +25 05 11.8 11.7 U Ari 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 111959111528094592,2461231.8767,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 111959111528094592 20260710.3767 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.76 02:31:16.94 +18:49:19.8
153.42022 -38.06800 galactic Ari Second-epoch detections are separated by 0.7" and 9.4 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 86213879260796416 | 02:31:16.87 +18:49:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.623+/-0.031 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:16.94 +18:49:19.8: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:16.94 +18:49:19.8: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 10.3767* 02 31 16.94 +18 49 19.8 11.8 U Ari 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 86213879260796416,2461231.8767,11.76,0.05,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 86213879260796416 20260710.3767 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 10.3767 2461231.8767 11.76 02:49:58.79 +21:37:05.7
156.36296 -33.44667 galactic Ari Second-epoch detections are separated by 1.6" and 9.4 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 85497032039092352 | 02:49:58.76 +21:37:06.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.457+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:58.79 +21:37:05.7: 12.66 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:58.79 +21:37:05.7: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 49 58.79 +21 37 05.7 11.8 U Ari 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 85497032039092352,2461231.8767,11.76,0.05,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 85497032039092352 20260710.3767 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 10.3767 2461231.8767 11.76 03:00:15.12 +23:42:20.9
157.39040 -30.41143 galactic Ari Second-epoch detections are separated by 1.7" and 9.4 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 110224430072661504 | 03:00:15.17 +23:42:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.466+/-0.030 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:15.12 +23:42:20.9: 12.66 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:15.12 +23:42:20.9: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 00 15.12 +23 42 20.9 11.8 U Ari 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 110224430072661504,2461231.8767,11.76,0.05,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 110224430072661504 20260710.3767 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 10.3767 2461231.8767 11.70 02:51:26.18 +22:25:55.8
156.19264 -32.57718 galactic Ari Second-epoch detections are separated by 1.3" and 9.3 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 109627013005838336 | 02:51:26.16 +22:25:56.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.764+/-0.031 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:26.18 +22:25:55.8: 12.65 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:26.18 +22:25:55.8: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 10.3767* 02 51 26.18 +22 25 55.8 11.7 U Ari 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 109627013005838336,2461231.8767,11.70,0.05,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
Gaia DR3 109627013005838336 20260710.3767 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 10.3767 2461231.8767 11.73 02:55:45.89 +23:03:50.2
156.79077 -31.51041 galactic Ari Second-epoch detections are separated by 0.9" and 9.1 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 110127604329910784 | 02:55:45.85 +23:03:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.728+/-0.032 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:45.89 +23:03:50.2: 12.65 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:45.89 +23:03:50.2: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 10.3767* 02 55 45.89 +23 03 50.2 11.7 U Ari 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 110127604329910784,2461231.8767,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 110127604329910784 20260710.3767 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.72 02:31:14.76 +18:39:37.6
153.50879 -38.21420 galactic Ari Second-epoch detections are separated by 2.1" and 9.2 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 86157632369148544 | 02:31:14.72 +18:39:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.836+/-0.029 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:14.76 +18:39:37.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:14.76 +18:39:37.6: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 10.3767* 02 31 14.76 +18 39 37.6 11.7 U Ari 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 86157632369148544,2461231.8767,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 86157632369148544 20260710.3767 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.66 03:04:40.66 +24:47:38.0
157.66273 -28.94666 galactic Ari Second-epoch detections are separated by 0.8" and 9.1 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 111810265141497600 | 03:04:40.56 +24:47:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.336+/-0.027 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:40.66 +24:47:38.0: 12.65 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:40.66 +24:47:38.0: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 10.3767* 03 04 40.66 +24 47 38.0 11.7 U Ari 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 111810265141497600,2461231.8767,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 111810265141497600 20260710.3767 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.05 02:55:13.20 +22:39:57.3
156.91872 -31.91332 galactic Ari Second-epoch detections are separated by 1.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:55:13.20 +22:39:57.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.680+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:13.20 +22:39:57.3: 13.32 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:13.20 +22:39:57.3: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 55 13.20 +22 39 57.3 12.1 U Ari 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,2461231.8767,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.39 02:51:09.05 +20:14:24.3
157.52749 -34.46704 galactic Ari Second-epoch detections are separated by 1.7" and 9.4 pix
The object was found in VSX 1" ASAS J025109+2014.4
Type: MISC
# Max. Min./Amp. JD0 Period
12.670 V Y 0.580 V 2452760.10000 89.954037000000
The object was not found in astcheck.
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:09.05 +20:14:24.3: 12.63 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:09.05 +20:14:24.3: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 10.3767* 02 51 09.05 +20 14 24.3 11.4 U Ari 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
ASAS J025109+2014.4,2461231.8767,11.39,0.05,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
ASAS J025109+2014.4 20260710.3767 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 10.3767 2461231.8767 12.06 02:56:39.79 +21:10:15.9
158.21704 -32.98395 galactic Ari Second-epoch detections are separated by 1.3" and 9.4 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 | 02:56:39.79 +21:10:15.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.820+/-0.028 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:39.79 +21:10:15.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:39.79 +21:10:15.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 39.79 +21 10 15.9 12.1 U Ari 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,2461231.8767,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 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 10.3767 2461231.8767 11.94 02:52:05.18 +22:04:50.4
156.56552 -32.79554 galactic Ari Second-epoch detections are separated by 0.3" and 9.2 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 | 02:52:05.18 +22:04:50.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.828+/-0.030 (M)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:05.18 +22:04:50.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:05.18 +22:04:50.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 10.3767* 02 52 05.18 +22 04 50.4 11.9 U Ari 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,2461231.8767,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.00 02:49:47.56 +20:19:44.2
157.14339 -34.56277 galactic Ari Second-epoch detections are separated by 2.9" and 9.4 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 | 02:49:47.56 +20:19:44.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.449+/-0.028 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:47.56 +20:19:44.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:47.56 +20:19:44.2: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 49 47.56 +20 19 44.2 12.0 U Ari 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,2461231.8767,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.92 02:56:00.99 +22:18:26.3
157.33010 -32.11526 galactic Ari Second-epoch detections are separated by 1.8" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:56:00.99 +22:18:26.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.686+/-0.031 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:00.99 +22:18:26.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:00.99 +22:18:26.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 10.3767* 02 56 00.99 +22 18 26.3 11.9 U Ari 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,2461231.8767,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 12.04 02:50:28.37 +21:22:38.5
156.63250 -33.59046 galactic Ari Second-epoch detections are separated by 0.5" and 9.3 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 | 02:50:28.37 +21:22:38.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.516+/-0.029 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:28.37 +21:22:38.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:28.37 +21:22:38.5: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 50 28.37 +21 22 38.5 12.0 U Ari 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,2461231.8767,12.04,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.81 02:29:12.20 +19:08:51.9
152.67492 -38.01310 galactic Ari Second-epoch detections are separated by 1.3" and 9.7 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 | 02:29:12.20 +19:08:51.9 (user input) | T | P | (position from user input) J-Ks=0.756+/-0.027 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:12.20 +19:08:51.9: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:12.20 +19:08:51.9: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 29 12.20 +19 08 51.9 11.8 U Ari 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,2461231.8767,11.81,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.82 02:28:54.16 +18:26:47.5
153.01393 -38.66584 galactic Ari Second-epoch detections are separated by 1.9" and 9.6 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 | 02:28:54.16 +18:26:47.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.449+/-0.030 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:54.16 +18:26:47.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:54.16 +18:26:47.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 10.3767* 02 28 54.16 +18 26 47.5 11.8 U Ari 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,2461231.8767,11.82,0.05,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 20260710.3767 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 10.3767 2461231.8767 11.91 03:02:54.79 +24:52:46.9
157.22758 -29.09777 galactic Ari Second-epoch detections are separated by 3.6" and 9.5 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 | 03:02:54.79 +24:52:46.9 (user input) | T | P | (position from user input) J-Ks=0.488+/-0.028 (K)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:54.79 +24:52:46.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:54.79 +24:52:46.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 03 02 54.79 +24 52 46.9 11.9 U Ari 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,2461231.8767,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3767 2461231.8767 11.93 02:56:09.10 +23:04:32.7
156.87115 -31.45247 galactic Ari Second-epoch detections are separated by 2.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:56:09.10 +23:04:32.7 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.032 (G)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:09.10 +23:04:32.7: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:09.10 +23:04:32.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3767* 02 56 09.10 +23 04 32.7 11.9 U Ari 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,2461231.8767,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3767 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461231.87695846 10.07.2026 09:02:39.211 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 17 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): 6883
Objects passed selection criteria: 6835
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 3862.25
Average stars matched: 3699.5 (95.7861 %)
Memory usage VmPeak: 113312 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 05:53:56 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461231.87695846 10.07.2026 09:02:39.211 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 162
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 26 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): 42640
Objects passed selection criteria: 42483
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 25115.5
Average stars matched: 23669.2 (94.2416 %)
Memory usage VmPeak: 146160 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 05:57:02 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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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: 2461231.87639127
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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
Saving wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits exists and is non-empty
Saving wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits to local_wcs_cache/
'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits exists and is non-empty
Saving wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits to local_wcs_cache/
'wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits' -> 'local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits'
wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits exists and is non-empty
Saving wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits to local_wcs_cache/
'wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits' -> 'local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (1st reference image)
verification OK: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:46:09.097 +22:00:02.05 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits (1st new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:08.624 +21:58:44.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:46:09.097 +22:00:02.05
Second-epoch image center 02:46:08.624 +21:58:44.77
Angular distance between the image centers 0.0215 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits (2nd new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:11.576 +21:58:06.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:46:09.097 +22:00:02.05
Second-epoch image center 02:46:11.576 +21:58:06.78
Angular distance between the image centers 0.0334 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 02:46:08.624 +21:58:44.77
Second-epoch second image center 02:46:11.576 +21:58:06.78
Angular distance between the image centers 0.01554 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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.StFjR2JRS2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits &> /tmp/tmp.vVk6egVuHP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits &> /tmp/tmp.W2iVsC4OWO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits &> /tmp/tmp.yWMTvyGCPh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
The reference image (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat) found
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat' -> 'wcsmag.cat'
Read 9126 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8271 to 50.3980 deg, Dec +16.4922 to +27.2905 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 32.8271 to 50.3980 deg, Dec 16.4922 to 27.2905 deg
Loaded 5488 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): 4334 out of 4603 total matches.
Matched with Tycho-2 4603 out of 9126 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.948500
a=0.000000 b=1.000000 c=22.948500
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9126 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8271 to 50.3980 deg, Dec +16.4922 to +27.2905 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 32.8271 to 50.3980 deg, Dec 16.4922 to 27.2905 deg
Loaded 5488 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): 4334 out of 4603 total matches.
Matched with Tycho-2 4603 out of 9126 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits:
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (aperture=6.0)
Read 9076 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.7981 to 50.3454 deg, Dec +16.4922 to +27.2893 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 32.7981 to 50.3454 deg, Dec 16.4922 to 27.2893 deg
Loaded 5483 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): 4341 out of 4608 total matches.
Matched with Tycho-2 4608 out of 9076 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits:
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
2.0 pix Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
2.0 pix wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
2.0 pix wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Limiting magnitude estimates:
15.4 mag. Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
15.4 mag. Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
11.7 mag. fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
11.6 mag. fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 9.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.StFjR2JRS2 (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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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=637, bad_region=2094, passed=9126
Got 9126 stars (including 6525 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 9126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 7261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 7262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 7262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits N_match=973 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.316 n_q1=296 n_q2=184 n_q3=298 n_q4=195 worst_quadrant_to_overall_ratio=1.159
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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.vVk6egVuHP (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/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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=628, bad_region=2087, passed=9076
Got 9076 stars (including 6485 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 9076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 7231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 7231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 7231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits N_match=974 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.307 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.301 n_q1=299 n_q2=184 n_q3=298 n_q4=193 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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.W2iVsC4OWO (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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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=196, bad_region=328, passed=1061
Got 1061 stars (including 678 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat
util/solve_plate_with_UCAC5 got 1061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 642 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 641 matched stars entering correct_measured_positions(), 624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 641 matched stars entering correct_measured_positions(), 745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 642 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 640 stars left (next iteration limit 705)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits N_match=640 sigma_overall_arcsec=0.547 sigma_q1_arcsec=0.536 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.586 sigma_q4_arcsec=0.547 n_q1=185 n_q2=79 n_q3=223 n_q4=153 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits -region wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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.yWMTvyGCPh (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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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=158, bad_region=303, passed=1093
Got 1093 stars (including 734 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat
util/solve_plate_with_UCAC5 got 1093 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 699 matched stars entering correct_measured_positions(), 681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 699 matched stars entering correct_measured_positions(), 807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 533 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 698 matched stars entering correct_measured_positions(), 807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 698 matched stars entering correct_measured_positions(), 807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 698 stars left (next iteration limit 768)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits N_match=698 sigma_overall_arcsec=0.497 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.552 sigma_q4_arcsec=0.484 n_q1=204 n_q2=91 n_q3=253 n_q4=150 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits -region wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits sigma_overall=0.356 worst_q_ratio=1.159
ref2=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits sigma_overall=0.341 worst_q_ratio=1.115
new1=fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits sigma_overall=0.547 worst_q_ratio=1.071
new2=fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits sigma_overall=0.497 worst_q_ratio=1.111
reference average sigma_overall=0.3485 worst_q_ratio=1.137
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131_astrometric_residuals.png (973 matched stars from wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132_astrometric_residuals.png (974 matched stars from wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384_astrometric_residuals.png (640 matched stars from wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385_astrometric_residuals.png (698 matched stars from wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits'
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits'
Preparing the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Creating symlink local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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
Plate-solving the images
wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (1st reference image)
verification OK: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:46:09.097 +22:00:02.05 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits (1st new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:08.624 +21:58:44.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:46:09.097 +22:00:02.05
Second-epoch image center 02:46:08.624 +21:58:44.77
Angular distance between the image centers 0.0215 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits (2nd new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:11.576 +21:58:06.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:46:09.097 +22:00:02.05
Second-epoch image center 02:46:11.576 +21:58:06.78
Angular distance between the image centers 0.0334 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 02:46:08.624 +21:58:44.77
Second-epoch second image center 02:46:11.576 +21:58:06.78
Angular distance between the image centers 0.01554 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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.TC9XanQs1Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits &> /tmp/tmp.WcIMnDROSQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits &> /tmp/tmp.4sj2Chzl0Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits &> /tmp/tmp.CGZ0bp7ReP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
The reference image (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat) found
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat' -> 'wcsmag.cat'
Read 54392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8063 to 50.3979 deg, Dec +16.4766 to +27.2962 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 32.8063 to 50.3979 deg, Dec 16.4766 to 27.2962 deg
Loaded 5501 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): 4044 out of 4645 total matches.
Matched with Tycho-2 4645 out of 54392 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.822150
a=0.000000 b=1.000000 c=22.822150
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 54392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8063 to 50.3979 deg, Dec +16.4766 to +27.2962 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 32.8063 to 50.3979 deg, Dec 16.4766 to 27.2962 deg
Loaded 5501 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): 4044 out of 4645 total matches.
Matched with Tycho-2 4645 out of 54392 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits:
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (aperture=4.6)
Read 54252 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.7981 to 50.3818 deg, Dec +16.4764 to +27.2953 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 32.7981 to 50.3818 deg, Dec 16.4764 to 27.2953 deg
Loaded 5500 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): 4042 out of 4646 total matches.
Matched with Tycho-2 4646 out of 54252 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits:
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 133 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
1.9 pix Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
2.1 pix fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
2.2 pix fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
1.9 pix wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
1.9 pix wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Limiting magnitude estimates:
15.6 mag. Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
15.6 mag. Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
12.3 mag. fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
12.3 mag. fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
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.TC9XanQs1Y (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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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=10, blended=2743, bad_region=10132, passed=54382
Got 54382 stars (including 41937 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 54382 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits N_match=972 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.304 sigma_q4_arcsec=0.287 n_q1=299 n_q2=182 n_q3=297 n_q4=194 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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.WcIMnDROSQ (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/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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=5, blended=2775, bad_region=10166, passed=54247
Got 54247 stars (including 41735 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 54247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 45263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 45263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 45263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits N_match=971 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.265 n_q1=298 n_q2=181 n_q3=300 n_q4=192 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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.4sj2Chzl0Y (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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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=18, no_mag_err=0, low_SNR=14, blended=379, bad_region=1136, passed=7346
Got 7346 stars (including 6089 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat
util/solve_plate_with_UCAC5 got 7346 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 6226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 6224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 6224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits N_match=952 sigma_overall_arcsec=0.517 sigma_q1_arcsec=0.504 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.538 sigma_q4_arcsec=0.505 n_q1=280 n_q2=108 n_q3=342 n_q4=222 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits -region wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.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.CGZ0bp7ReP (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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.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=23, no_mag_err=0, low_SNR=12, blended=394, bad_region=1179, passed=7645
Got 7645 stars (including 6338 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat
util/solve_plate_with_UCAC5 got 7645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 6480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 6480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 6480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits N_match=957 sigma_overall_arcsec=0.493 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.525 sigma_q4_arcsec=0.505 n_q1=291 n_q2=124 n_q3=333 n_q4=209 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits -region wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-01-50_20.00sec_4.90C_LIGHT_0384.fits
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Ari-03-Q2b1x1_055103_TTUQ2b1x1_2189486_vif3lQU9/wcs_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385.fits
Preparing the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:06.25 +19:29:33.8: 12.42 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:01:56.83 +23:38:27.8: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:32.89 +18:19:41.3: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:19.15 +18:04:19.3: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:16.64 +20:21:30.8: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:58.97 +21:58:59.1: 12.72 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:18.69 +20:52:04.5: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:35.44 +21:57:40.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:08.81 +20:33:20.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:17.40 +17:58:32.1: 12.64 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:01:56.83 +23:38:27.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 03:01:56.83 +23:38:27.8: ref_mag=12.87 +/- 0.01 new_mean_mag=11.7768 delta=1.09 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:06.25 +19:29:33.8: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 02:33:06.25 +19:29:33.8: ref_mag=12.41 +/- 0.01 new_mean_mag=12.1082 delta=0.31 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:32.89 +18:19:41.3: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:19.15 +18:04:19.3: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:32.89 +18:19:41.3: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6394 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:19.15 +18:04:19.3: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6841 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:08.81 +20:33:20.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 02:53:08.81 +20:33:20.9: ref_mag=13.01 +/- 0.01 new_mean_mag=11.9992 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:17.40 +17:58:32.1: 12.60 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:16.64 +20:21:30.8: 13.06 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:35.44 +21:57:40.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:16.64 +20:21:30.8: ref_mag=13.07 +/- 0.01 new_mean_mag=11.9331 delta=1.13 (need > 0.90)
Forced photometry filter KEPT candidate at 02:27:17.40 +17:58:32.1: ref_mag=12.62 +/- 0.01 new_mean_mag=11.4811 delta=1.14 (need > 0.90)
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 02:54:35.44 +21:57:40.9: ref_mag=13.08 +/- 0.01 new_mean_mag=12.0564 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:18.69 +20:52:04.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:18.69 +20:52:04.5: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7626 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:58.97 +21:58:59.1: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 02:53:58.97 +21:58:59.1: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6725 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:43.08 +25:02:52.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:43.08 +25:02:52.9: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 03:02:43.08 +25:02:52.9: ref_mag=12.79 +/- 0.01 new_mean_mag=11.7349 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:10.58 +18:39:04.0: 13.13 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:10.58 +18:39:04.0: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 02:27:10.58 +18:39:04.0: ref_mag=13.11 +/- 0.02 new_mean_mag=11.8009 delta=1.31 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:29.77 +18:16:03.7: 12.33 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:29.77 +18:16:03.7: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:29.77 +18:16:03.7: ref_mag=12.30 +/- 0.01 new_mean_mag=11.3901 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:09.00 +19:35:17.0: 12.35 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:53.95 +21:07:47.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:32.10 +19:13:01.7: 12.40 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:09.00 +19:35:17.0: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:09.00 +19:35:17.0: ref_mag=12.34 +/- 0.01 new_mean_mag=11.4074 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:53.95 +21:07:47.7: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:32.10 +19:13:01.7: 12.38 +/- 0.01 detection
Forced photometry filter KEPT candidate at 02:52:53.95 +21:07:47.7: ref_mag=12.83 +/- 0.01 new_mean_mag=11.9008 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:32.10 +19:13:01.7: ref_mag=12.39 +/- 0.01 new_mean_mag=11.4112 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:46:40.96 +19:00:22.4: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:01.46 +22:19:39.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:01.46 +22:19:39.0: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:01.46 +22:19:39.0: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9006 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:42.46 +19:09:36.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:06.80 +23:28:44.5: 13.23 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:46:40.96 +19:00:22.4: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 02:46:40.96 +19:00:22.4: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1514 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:42.46 +19:09:36.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:06.80 +23:28:44.5: 13.29 +/- 0.02 detection
Forced photometry filter KEPT candidate at 02:29:42.46 +19:09:36.5: ref_mag=12.86 +/- 0.01 new_mean_mag=11.7002 delta=1.16 (need > 0.90)
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 02:57:06.80 +23:28:44.5: ref_mag=13.26 +/- 0.02 new_mean_mag=12.0603 delta=1.20 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:27.12 +20:26:14.0: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:27.12 +20:26:14.0: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 02:52:27.12 +20:26:14.0: ref_mag=13.00 +/- 0.01 new_mean_mag=12.0436 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:59:34.37 +23:23:01.8: 12.99 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:59:34.37 +23:23:01.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 02:59:34.37 +23:23:01.8: ref_mag=12.98 +/- 0.01 new_mean_mag=11.9026 delta=1.08 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:04.00 +21:46:00.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:04.00 +21:46:00.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 02:51:04.00 +21:46:00.8: ref_mag=12.99 +/- 0.01 new_mean_mag=11.9384 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:36.12 +18:58:03.3: 12.57 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:46.21 +18:33:54.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:36.12 +18:58:03.3: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:36.12 +18:58:03.3: ref_mag=12.57 +/- 0.01 new_mean_mag=11.6391 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:46.21 +18:33:54.1: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 02:29:46.21 +18:33:54.1: ref_mag=13.27 +/- 0.02 new_mean_mag=11.9769 delta=1.29 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:14.10 +18:32:32.1: 12.59 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:14.10 +18:32:32.1: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:14.10 +18:32:32.1: ref_mag=12.58 +/- 0.01 new_mean_mag=11.5575 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:52.26 +17:59:57.8: 12.58 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:52.26 +17:59:57.8: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:52.26 +17:59:57.8: ref_mag=12.58 +/- 0.01 new_mean_mag=11.6176 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:37.01 +22:52:55.8: 13.29 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:24.87 +18:57:20.1: 12.02 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:36.37 +21:14:36.0: 12.57 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:37.01 +22:52:55.8: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 02:57:37.01 +22:52:55.8: ref_mag=13.26 +/- 0.02 new_mean_mag=12.0670 delta=1.20 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:17.79 +22:24:50.6: 13.29 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:24.87 +18:57:20.1: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:24.87 +18:57:20.1: ref_mag=12.02 +/- 0.01 new_mean_mag=11.0717 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:36.37 +21:14:36.0: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 02:50:36.37 +21:14:36.0: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6443 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:17.79 +22:24:50.6: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 02:56:17.79 +22:24:50.6: ref_mag=13.30 +/- 0.02 new_mean_mag=12.0514 delta=1.25 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:08.49 +19:34:38.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:08.49 +19:34:38.8: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:08.49 +19:34:38.8: ref_mag=13.00 +/- 0.01 new_mean_mag=11.8697 delta=1.13 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:08.42 +17:47:32.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:08.42 +17:47:32.8: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:08.42 +17:47:32.8: ref_mag=12.99 +/- 0.01 new_mean_mag=11.7139 delta=1.27 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:25.21 +18:05:46.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:40.89 +20:51:37.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:25.21 +18:05:46.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 02:27:25.21 +18:05:46.8: ref_mag=12.98 +/- 0.01 new_mean_mag=11.7284 delta=1.25 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:40.89 +20:51:37.7: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 02:49:40.89 +20:51:37.7: ref_mag=12.98 +/- 0.01 new_mean_mag=11.9661 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:48:45.83 +20:45:32.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:12.48 +23:33:18.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:48:45.83 +20:45:32.2: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 02:48:45.83 +20:45:32.2: ref_mag=12.99 +/- 0.01 new_mean_mag=11.9644 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:12.48 +23:33:18.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 02:57:12.48 +23:33:18.8: ref_mag=12.96 +/- 0.01 new_mean_mag=11.9117 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:00.60 +23:46:00.2: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:35.23 +22:27:31.7: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:00.60 +23:46:00.2: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 03:02:00.60 +23:46:00.2: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5972 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:35.23 +22:27:31.7: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 02:53:35.23 +22:27:31.7: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6075 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:49.45 +19:31:49.0: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:59.79 +18:29:42.7: 12.54 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:49.45 +19:31:49.0: 12.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:49.45 +19:31:49.0: ref_mag=12.57 +/- 0.01 new_mean_mag=11.4796 delta=1.09 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:59.79 +18:29:42.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 02:27:59.79 +18:29:42.7: ref_mag=12.55 +/- 0.01 new_mean_mag=11.3978 delta=1.15 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:48.92 +23:33:35.0: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:48.92 +23:33:35.0: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 02:54:48.92 +23:33:35.0: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6392 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:16.08 +23:07:39.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:16.08 +23:07:39.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 02:53:16.08 +23:07:39.0: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5883 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:13.03 +18:34:05.4: 13.23 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:13.03 +18:34:05.4: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 02:27:13.03 +18:34:05.4: ref_mag=13.24 +/- 0.02 new_mean_mag=11.8155 delta=1.42 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:13.86 +19:27:59.3: 13.24 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:13.86 +19:27:59.3: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 02:29:13.86 +19:27:59.3: ref_mag=13.21 +/- 0.02 new_mean_mag=11.8877 delta=1.32 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:12.57 +21:49:55.4: 13.22 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:12.57 +21:49:55.4: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.01
Forced photometry filter KEPT candidate at 02:51:12.57 +21:49:55.4: ref_mag=13.22 +/- 0.01 new_mean_mag=11.9967 delta=1.23 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:06.42 +22:49:48.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:06.42 +22:49:48.3: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 02:55:06.42 +22:49:48.3: ref_mag=12.98 +/- 0.01 new_mean_mag=11.8048 delta=1.18 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:48:36.57 +19:31:40.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:30.94 +23:08:45.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:48:36.57 +19:31:40.9: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 02:48:36.57 +19:31:40.9: ref_mag=12.95 +/- 0.01 new_mean_mag=12.0258 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:30.94 +23:08:45.4: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 02:54:30.94 +23:08:45.4: ref_mag=12.91 +/- 0.01 new_mean_mag=11.9369 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:34.49 +22:04:48.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:28.63 +19:37:44.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:33.47 +18:46:22.6: 11.84 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:34.49 +22:04:48.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 02:55:34.49 +22:04:48.9: ref_mag=12.94 +/- 0.01 new_mean_mag=11.9536 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:28.63 +19:37:44.4: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:28.63 +19:37:44.4: ref_mag=12.89 +/- 0.01 new_mean_mag=11.7053 delta=1.19 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:33.47 +18:46:22.6: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Forced photometry filter KEPT candidate at 02:28:33.47 +18:46:22.6: ref_mag=11.83 +/- 0.00 new_mean_mag=10.9070 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:02.59 +21:37:56.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:02.59 +21:37:56.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:02.59 +21:37:56.6: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8749 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:52.83 +20:58:13.7: 12.91 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:52.83 +20:58:13.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 02:49:52.83 +20:58:13.7: ref_mag=12.91 +/- 0.01 new_mean_mag=11.9346 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:30.72 +18:15:36.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:30.72 +18:15:36.8: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:30.72 +18:15:36.8: ref_mag=12.94 +/- 0.01 new_mean_mag=11.7840 delta=1.15 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:48.31 +20:53:33.4: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:48.31 +20:53:33.4: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:48.31 +20:53:33.4: ref_mag=12.89 +/- 0.01 new_mean_mag=11.8111 delta=1.08 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:31.84 +19:33:46.3: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:31.84 +19:33:46.3: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:31.84 +19:33:46.3: ref_mag=12.90 +/- 0.01 new_mean_mag=11.7747 delta=1.13 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:21.31 +20:14:14.3: 12.50 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:40.58 +22:49:15.5: 13.21 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:21.31 +20:14:14.3: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:21.31 +20:14:14.3: ref_mag=12.51 +/- 0.01 new_mean_mag=11.5631 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:40.58 +22:49:15.5: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.01
Forced photometry filter KEPT candidate at 02:53:40.58 +22:49:15.5: ref_mag=13.21 +/- 0.01 new_mean_mag=12.0222 delta=1.18 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:15.94 +21:57:30.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:59:38.51 +23:05:13.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:19.34 +23:20:15.6: 12.47 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:15.94 +21:57:30.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:59:38.51 +23:05:13.2: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.01
Forced photometry filter KEPT candidate at 02:52:15.94 +21:57:30.0: ref_mag=13.17 +/- 0.01 new_mean_mag=12.0103 delta=1.16 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 02:59:38.51 +23:05:13.2: ref_mag=13.20 +/- 0.02 new_mean_mag=11.9961 delta=1.21 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:19.34 +23:20:15.6: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:19.34 +23:20:15.6: ref_mag=12.49 +/- 0.01 new_mean_mag=11.5589 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:08.58 +20:04:49.8: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:08.58 +20:04:49.8: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:08.58 +20:04:49.8: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4760 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:14.53 +19:32:29.3: 12.44 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:14.53 +19:32:29.3: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:14.53 +19:32:29.3: ref_mag=12.44 +/- 0.01 new_mean_mag=11.4230 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:42.97 +18:46:27.0: 12.43 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:42.97 +18:46:27.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:42.97 +18:46:27.0: ref_mag=12.42 +/- 0.01 new_mean_mag=11.3947 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:21.06 +18:44:38.5: 12.41 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:21.06 +18:44:38.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:21.06 +18:44:38.5: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4983 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:09.44 +22:24:59.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:09.44 +22:24:59.0: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:09.44 +22:24:59.0: ref_mag=13.15 +/- 0.01 new_mean_mag=11.9490 delta=1.21 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:15.18 +19:53:45.4: 13.17 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:41.93 +20:05:42.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:15.18 +19:53:45.4: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 02:31:15.18 +19:53:45.4: ref_mag=13.21 +/- 0.02 new_mean_mag=11.9821 delta=1.22 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:41.93 +20:05:42.6: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:41.93 +20:05:42.6: ref_mag=12.83 +/- 0.01 new_mean_mag=11.7871 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:56.11 +20:24:47.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:25.58 +18:07:17.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:48:43.22 +20:12:41.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:56.11 +20:24:47.8: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 02:51:56.11 +20:24:47.8: ref_mag=12.86 +/- 0.01 new_mean_mag=11.9313 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:25.58 +18:07:17.2: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 02:27:25.58 +18:07:17.2: ref_mag=12.37 +/- 0.01 new_mean_mag=11.3049 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:48:43.22 +20:12:41.1: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 02:48:43.22 +20:12:41.1: ref_mag=12.29 +/- 0.01 new_mean_mag=11.2844 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:28.65 +18:56:39.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:28.65 +18:56:39.4: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 02:28:28.65 +18:56:39.4: ref_mag=13.14 +/- 0.02 new_mean_mag=11.8672 delta=1.27 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:24.52 +18:15:11.2: 13.13 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:24.52 +18:15:11.2: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 02:27:24.52 +18:15:11.2: ref_mag=13.14 +/- 0.02 new_mean_mag=11.8355 delta=1.30 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:05.73 +22:57:22.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:05.73 +22:57:22.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 02:53:05.73 +22:57:22.4: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8455 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:03:41.47 +24:55:39.4: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:03:41.47 +24:55:39.4: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 03:03:41.47 +24:55:39.4: ref_mag=12.88 +/- 0.01 new_mean_mag=11.8240 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:21.82 +22:30:29.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:21.82 +22:30:29.6: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 02:50:21.82 +22:30:29.6: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8791 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:32:22.04 +18:29:35.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:32:22.04 +18:29:35.3: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 02:32:22.04 +18:29:35.3: ref_mag=12.85 +/- 0.01 new_mean_mag=11.7818 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:50.02 +19:14:10.1: 13.13 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:50.02 +19:14:10.1: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 02:28:50.02 +19:14:10.1: ref_mag=13.13 +/- 0.02 new_mean_mag=11.9551 delta=1.17 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:19.03 +23:32:13.3: 12.83 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:19.03 +23:32:13.3: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:19.03 +23:32:13.3: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8770 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:18.15 +21:55:47.4: 12.82 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:42.75 +23:23:52.6: 12.82 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:18.15 +21:55:47.4: 12.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 02:50:18.15 +21:55:47.4: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8292 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:42.75 +23:23:52.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 03:00:42.75 +23:23:52.6: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8490 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:42.50 +22:27:25.2: 12.82 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:42.50 +22:27:25.2: 12.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 02:55:42.50 +22:27:25.2: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8566 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:46.13 +20:07:50.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:02.28 +20:00:35.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:46.13 +20:07:50.1: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:46.13 +20:07:50.1: ref_mag=12.79 +/- 0.01 new_mean_mag=11.6935 delta=1.10 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:02.28 +20:00:35.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:02.28 +20:00:35.7: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7777 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:20.06 +18:40:07.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:20.06 +18:40:07.5: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:20.06 +18:40:07.5: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7823 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:18.73 +22:57:00.0: 12.78 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:18.73 +22:57:00.0: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 02:52:18.73 +22:57:00.0: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7800 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:37.30 +23:21:34.6: 12.80 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:37.30 +23:21:34.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:37.30 +23:21:34.6: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8064 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:05:01.43 +24:56:46.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:05:01.43 +24:56:46.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 03:05:01.43 +24:56:46.5: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8136 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:13.32 +24:22:02.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:13.32 +24:22:02.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 03:04:13.32 +24:22:02.2: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7986 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:46.30 +20:01:14.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:53.76 +18:26:16.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:46.30 +20:01:14.7: 12.76 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:53.76 +18:26:16.9: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:46.30 +20:01:14.7: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8211 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:53.76 +18:26:16.9: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7861 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:16.30 +19:55:45.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:16.30 +19:55:45.8: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 02:31:16.30 +19:55:45.8: ref_mag=13.12 +/- 0.02 new_mean_mag=11.8830 delta=1.24 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:58:18.32 +22:31:40.7: 12.76 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:26.15 +19:16:05.3: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:58:18.32 +22:31:40.7: 12.75 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:26.15 +19:16:05.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 02:58:18.32 +22:31:40.7: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7281 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 02:31:26.15 +19:16:05.3: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8336 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:01.35 +20:47:09.6: 12.74 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:01.35 +20:47:09.6: 12.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 02:50:01.35 +20:47:09.6: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7825 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:46.11 +25:12:30.3: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:46.11 +25:12:30.3: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 03:04:46.11 +25:12:30.3: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7184 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:49.20 +24:37:31.6: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:49.20 +24:37:31.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 03:02:49.20 +24:37:31.6: ref_mag=12.73 +/- 0.01 new_mean_mag=11.8019 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:01.86 +19:56:30.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:01.86 +19:56:30.6: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:01.86 +19:56:30.6: ref_mag=13.12 +/- 0.01 new_mean_mag=11.8953 delta=1.22 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:30.19 +21:14:03.8: 12.71 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:30.19 +21:14:03.8: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:30.19 +21:14:03.8: ref_mag=12.69 +/- 0.01 new_mean_mag=11.7495 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:01.93 +18:43:33.7: 12.71 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:01.93 +18:43:33.7: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:01.93 +18:43:33.7: ref_mag=12.72 +/- 0.01 new_mean_mag=11.6864 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:24.89 +20:11:35.0: 12.70 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:01:53.91 +24:08:51.3: 12.74 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:24.89 +20:11:35.0: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 02:49:24.89 +20:11:35.0: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6673 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:01:53.91 +24:08:51.3: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 03:01:53.91 +24:08:51.3: ref_mag=12.71 +/- 0.01 new_mean_mag=11.6732 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:40.63 +18:49:53.8: 12.25 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:40.63 +18:49:53.8: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:40.63 +18:49:53.8: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2119 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:13.42 +18:36:47.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:27:49.85 +18:34:08.4: 12.20 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:13.42 +18:36:47.5: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 02:27:13.42 +18:36:47.5: ref_mag=12.23 +/- 0.01 new_mean_mag=11.2395 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:27:49.85 +18:34:08.4: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 02:27:49.85 +18:34:08.4: ref_mag=12.20 +/- 0.01 new_mean_mag=11.1430 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:46.33 +20:53:17.1: 13.10 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:46.33 +20:53:17.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Forced photometry filter KEPT candidate at 02:50:46.33 +20:53:17.1: ref_mag=13.11 +/- 0.01 new_mean_mag=12.0518 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:17.58 +18:57:25.4: 12.70 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:17.58 +18:57:25.4: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:17.58 +18:57:25.4: ref_mag=12.71 +/- 0.01 new_mean_mag=11.6707 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:59.23 +21:20:47.7: 12.70 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:59.23 +21:20:47.7: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:59.23 +21:20:47.7: ref_mag=12.70 +/- 0.01 new_mean_mag=11.6847 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:22.95 +19:07:52.9: 13.61 +/- 0.03 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:22.95 +19:07:52.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Forced photometry filter KEPT candidate at 02:28:22.95 +19:07:52.9: ref_mag=13.56 +/- 0.02 new_mean_mag=12.0930 delta=1.47 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:19.66 +21:35:48.2: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:19.66 +21:35:48.2: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:19.66 +21:35:48.2: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7724 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:07.53 +23:04:39.9: 12.68 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:07.53 +23:04:39.9: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 02:55:07.53 +23:04:39.9: ref_mag=12.66 +/- 0.01 new_mean_mag=11.7206 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:26.67 +25:44:22.2: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:26.67 +25:44:22.2: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 03:04:26.67 +25:44:22.2: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6696 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:39.28 +25:05:11.8: 12.68 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:39.28 +25:05:11.8: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 03:04:39.28 +25:05:11.8: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6757 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:16.94 +18:49:19.8: 12.67 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:16.94 +18:49:19.8: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:16.94 +18:49:19.8: ref_mag=12.69 +/- 0.01 new_mean_mag=11.7349 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:58.79 +21:37:05.7: 12.66 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:58.79 +21:37:05.7: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 02:49:58.79 +21:37:05.7: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6901 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:15.12 +23:42:20.9: 12.66 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:15.12 +23:42:20.9: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 03:00:15.12 +23:42:20.9: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7471 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:26.18 +22:25:55.8: 12.65 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:26.18 +22:25:55.8: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 02:51:26.18 +22:25:55.8: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6966 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:45.89 +23:03:50.2: 12.65 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:45.89 +23:03:50.2: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 02:55:45.89 +23:03:50.2: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6953 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:14.76 +18:39:37.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:14.76 +18:39:37.6: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:14.76 +18:39:37.6: ref_mag=12.65 +/- 0.01 new_mean_mag=11.7231 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:04:40.66 +24:47:38.0: 12.65 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:04:40.66 +24:47:38.0: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 03:04:40.66 +24:47:38.0: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6667 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:55:13.20 +22:39:57.3: 13.32 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:55:13.20 +22:39:57.3: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 02:55:13.20 +22:39:57.3: ref_mag=13.29 +/- 0.02 new_mean_mag=12.0486 delta=1.24 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:09.05 +20:14:24.3: 12.63 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:09.05 +20:14:24.3: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 02:51:09.05 +20:14:24.3: ref_mag=12.61 +/- 0.01 new_mean_mag=11.3938 delta=1.21 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:39.79 +21:10:15.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:39.79 +21:10:15.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:39.79 +21:10:15.9: ref_mag=13.07 +/- 0.01 new_mean_mag=12.0658 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:52:05.18 +22:04:50.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:52:05.18 +22:04:50.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 02:52:05.18 +22:04:50.4: ref_mag=13.02 +/- 0.01 new_mean_mag=11.9384 delta=1.08 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:49:47.56 +20:19:44.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:49:47.56 +20:19:44.2: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 02:49:47.56 +20:19:44.2: ref_mag=13.03 +/- 0.01 new_mean_mag=12.0025 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:00.99 +22:18:26.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:00.99 +22:18:26.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:00.99 +22:18:26.3: ref_mag=13.02 +/- 0.01 new_mean_mag=11.9009 delta=1.12 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:28.37 +21:22:38.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:28.37 +21:22:38.5: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 02:50:28.37 +21:22:38.5: ref_mag=13.03 +/- 0.01 new_mean_mag=12.0163 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:29:12.20 +19:08:51.9: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:29:12.20 +19:08:51.9: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:12.20 +19:08:51.9: ref_mag=13.03 +/- 0.01 new_mean_mag=11.7761 delta=1.26 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:54.16 +18:26:47.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:54.16 +18:26:47.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 02:28:54.16 +18:26:47.5: ref_mag=13.02 +/- 0.01 new_mean_mag=11.8224 delta=1.20 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:54.79 +24:52:46.9: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:54.79 +24:52:46.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 03:02:54.79 +24:52:46.9: ref_mag=12.99 +/- 0.01 new_mean_mag=11.8786 delta=1.11 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:09.10 +23:04:32.7: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:09.10 +23:04:32.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 02:56:09.10 +23:04:32.7: ref_mag=13.00 +/- 0.01 new_mean_mag=11.9347 delta=1.07 (need > 0.90)
Adding exclusion_list_local.txt__out08404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40594.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out40724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42037.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out42526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42594.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out43084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43415.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out43808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44056.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out44853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46514.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out48500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48533.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out48778.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out50332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53865.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 200s
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: 66s
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Considering the candidate 67544_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
The candidate 67544_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385 did not pass the final checks
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Considering the candidate 51474_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 51474_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 53126_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 53126_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 39045_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 39045_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 39360_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 39360_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 41021_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 41021_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 29983_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 29983_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 29853_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 29853_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 39264_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 39264_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 20705_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 20705_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 12571_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 12571_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43084_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43084_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 40724_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 40724_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48654_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48654_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 34040_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 34040_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 46514_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 46514_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 28156_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 28156_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 45544_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 45544_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 45873_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 45873_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 21896_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 21896_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 53865_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 53865_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 22317_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 22317_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 30976_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 30976_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 44894_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 44894_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42570_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42570_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42037_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42037_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 38942_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 38942_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 44479_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 44479_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 25284_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 25284_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 33508_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 33508_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27752_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27752_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48533_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48533_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48794_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48794_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 39868_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 39868_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 39084_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 39084_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42526_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42526_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 21467_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 21467_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 19981_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 19981_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27577_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27577_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48207_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48207_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 41962_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 41962_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 21492_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 21492_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 23956_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 23956_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42594_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42594_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 47792_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 47792_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 30670_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 30670_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25594_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 25594_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48500_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48500_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 23894_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 23894_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 29381_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 29381_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43793_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43793_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48778_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48778_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 31795_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 31795_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 34902_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 34902_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 40772_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 40772_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 40100_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 40100_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48574_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48574_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 52463_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 52463_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 25700_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 25700_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 30080_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 30080_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 23969_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 23969_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 22680_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 22680_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 51410_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 51410_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 48279_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 48279_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43796_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43796_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43683_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43683_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27730_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27730_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 50332_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 50332_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 51656_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 51656_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 53672_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 53672_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 39524_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 39524_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 52474_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 52474_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 44853_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 44853_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 40701_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 40701_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 24974_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 24974_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 13216_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 13216_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27456_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27456_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42222_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42222_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 46512_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 46512_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 21559_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 21559_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 30210_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 30210_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 22187_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 22187_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27520_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27520_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 18832_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
The candidate 18832_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385 did not pass the final checks
**** FOUND 02:55:37.21 +23:59:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51690_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 51690_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 51042_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 51042_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43147_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43147_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 25043_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 25043_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 22542_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 22542_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 13050_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 13050_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 16478_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 16478_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 51193_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 51193_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 41512_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 41512_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 50772_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 50772_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27085_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27085_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 46682_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 46682_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 41372_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 41372_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 11464_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 11464_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 15052_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 15052_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 50120_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 50120_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 33653_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 33653_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43415_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43415_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 52339_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 52339_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 17849_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 17849_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 44056_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 44056_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42859_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42859_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 42621_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 42621_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 40594_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 40594_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 44841_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 44841_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 33142_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 33142_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 45947_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 45947_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 31946_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 31946_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 24196_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 24196_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 08404_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 08404_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 12233_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 12233_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43808_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43808_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 31721_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 31721_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 20401_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 20401_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 27765_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 27765_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 24225_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 24225_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 43108_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 43108_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 13979_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 13979_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 26498_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 26498_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 52509_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 52509_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 33692_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 33692_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 29455_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 29455_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 53037_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 53037_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 28269_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 28269_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 32893_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 32893_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 45850_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 45850_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 41872_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 41872_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 13595_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 13595_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
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Considering the candidate 24221_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
Preparing report for the candidate 24221_fd_Ari-03-Q2b1x1_2026-07-10_04-02-39_20.00sec_4.90C_LIGHT_0385
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 277s
Prepared the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:04:26.67 +25:44:22.2
03:04:46.11 +25:12:30.3
03:04:39.28 +25:05:11.8
03:02:43.08 +25:02:52.9
03:05:01.43 +24:56:46.5
03:03:41.47 +24:55:39.4
03:02:54.79 +24:52:46.9
03:04:40.66 +24:47:38.0
03:02:49.20 +24:37:31.6
03:04:13.32 +24:22:02.2
03:01:53.91 +24:08:51.3
03:02:00.60 +23:46:00.2
03:00:15.12 +23:42:20.9
03:01:56.83 +23:38:27.8
02:57:12.48 +23:33:18.8
02:54:48.92 +23:33:35.0
02:56:19.03 +23:32:13.3
02:57:06.80 +23:28:44.5
03:00:42.75 +23:23:52.6
02:59:34.37 +23:23:01.8
02:56:37.30 +23:21:34.6
02:56:19.34 +23:20:15.6
02:54:30.94 +23:08:45.4
02:53:16.08 +23:07:39.0
02:59:38.51 +23:05:13.2
02:55:07.53 +23:04:39.9
02:56:09.10 +23:04:32.7
02:55:45.89 +23:03:50.2
02:53:05.73 +22:57:22.4
02:52:18.73 +22:57:00.0
02:57:37.01 +22:52:55.8
02:55:06.42 +22:49:48.3
02:53:40.58 +22:49:15.5
02:55:13.20 +22:39:57.3
02:58:18.32 +22:31:40.7
02:50:21.82 +22:30:29.6
02:55:42.50 +22:27:25.2
02:53:35.23 +22:27:31.7
02:56:09.44 +22:24:59.0
02:56:17.79 +22:24:50.6
02:51:26.18 +22:25:55.8
02:56:01.46 +22:19:39.0
02:56:00.99 +22:18:26.3
02:55:34.49 +22:04:48.9
02:52:05.18 +22:04:50.4
02:53:58.97 +21:58:59.1
02:54:35.44 +21:57:40.9
02:52:15.94 +21:57:30.0
02:50:18.15 +21:55:47.4
02:51:12.57 +21:49:55.4
02:51:04.00 +21:46:00.8
02:49:58.79 +21:37:05.7
02:33:02.59 +21:37:56.6
02:33:19.66 +21:35:48.2
02:50:28.37 +21:22:38.5
02:31:59.23 +21:20:47.7
02:50:36.37 +21:14:36.0
02:30:30.19 +21:14:03.8
02:56:39.79 +21:10:15.9
02:52:53.95 +21:07:47.7
02:49:52.83 +20:58:13.7
02:28:52.26 +17:59:57.8
02:27:17.40 +17:58:32.1
02:49:40.89 +20:51:37.7
02:30:18.69 +20:52:04.5
02:29:19.15 +18:04:19.3
02:27:25.58 +18:07:17.2
02:27:25.21 +18:05:46.8
02:31:48.31 +20:53:33.4
02:50:46.33 +20:53:17.1
02:27:24.52 +18:15:11.2
02:29:29.77 +18:16:03.7
02:28:30.72 +18:15:36.8
02:29:32.89 +18:19:41.3
02:50:01.35 +20:47:09.6
02:31:53.76 +18:26:16.9
02:28:54.16 +18:26:47.5
02:27:59.79 +18:29:42.7
02:28:14.10 +18:32:32.1
02:32:22.04 +18:29:35.3
02:48:45.83 +20:45:32.2
02:29:46.21 +18:33:54.1
02:27:13.03 +18:34:05.4
02:27:49.85 +18:34:08.4
02:27:13.42 +18:36:47.5
02:27:10.58 +18:39:04.0
02:31:14.76 +18:39:37.6
02:31:20.06 +18:40:07.5
02:31:01.93 +18:43:33.7
02:30:21.06 +18:44:38.5
02:28:33.47 +18:46:22.6
02:29:42.97 +18:46:27.0
02:31:16.94 +18:49:19.8
02:28:40.63 +18:49:53.8
02:28:24.87 +18:57:20.1
02:31:17.58 +18:57:25.4
02:28:28.65 +18:56:39.4
02:31:36.12 +18:58:03.3
02:46:40.96 +19:00:22.4
02:29:12.20 +19:08:51.9
02:29:42.46 +19:09:36.5
02:28:22.95 +19:07:52.9
02:28:50.02 +19:14:10.1
02:28:32.10 +19:13:01.7
02:31:26.15 +19:16:05.3
02:29:13.86 +19:27:59.3
02:30:49.45 +19:31:49.0
02:29:14.53 +19:32:29.3
02:48:36.57 +19:31:40.9
02:30:08.49 +19:34:38.8
02:28:31.84 +19:33:46.3
02:30:09.00 +19:35:17.0
02:30:28.63 +19:37:44.4
02:28:08.42 +17:47:32.8
02:29:01.86 +19:56:30.6
02:31:15.18 +19:53:45.4
02:31:16.30 +19:55:45.8
02:29:02.28 +20:00:35.7
02:29:46.30 +20:01:14.7
02:30:08.58 +20:04:49.8
02:53:08.81 +20:33:20.9
02:29:41.93 +20:05:42.6
02:29:46.13 +20:07:50.1
02:49:24.89 +20:11:35.0
02:30:21.31 +20:14:14.3
02:48:43.22 +20:12:41.1
02:51:09.05 +20:14:24.3
02:49:47.56 +20:19:44.2
02:33:16.64 +20:21:30.8
02:51:56.11 +20:24:47.8
02:52:27.12 +20:26:14.0
########### Completed Ari-03-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 ####
02:53:08.81 +20:33:20.9
02:33:16.64 +20:21:30.8
02:27:17.40 +17:58:32.1
02:29:19.15 +18:04:19.3
02:29:32.89 +18:19:41.3
02:54:35.44 +21:57:40.9
02:53:58.97 +21:58:59.1
02:30:18.69 +20:52:04.5
03:01:56.83 +23:38:27.8
03:02:43.08 +25:02:52.9
02:27:10.58 +18:39:04.0
02:29:29.77 +18:16:03.7
02:30:09.00 +19:35:17.0
02:52:53.95 +21:07:47.7
02:28:32.10 +19:13:01.7
02:56:01.46 +22:19:39.0
02:46:40.96 +19:00:22.4
02:29:42.46 +19:09:36.5
02:57:06.80 +23:28:44.5
02:52:27.12 +20:26:14.0
02:59:34.37 +23:23:01.8
02:51:04.00 +21:46:00.8
02:31:36.12 +18:58:03.3
02:29:46.21 +18:33:54.1
02:28:14.10 +18:32:32.1
02:28:52.26 +17:59:57.8
02:28:24.87 +18:57:20.1
02:57:37.01 +22:52:55.8
02:50:36.37 +21:14:36.0
02:56:17.79 +22:24:50.6
02:30:08.49 +19:34:38.8
02:28:08.42 +17:47:32.8
02:27:25.21 +18:05:46.8
02:49:40.89 +20:51:37.7
02:48:45.83 +20:45:32.2
02:57:12.48 +23:33:18.8
03:02:00.60 +23:46:00.2
02:53:35.23 +22:27:31.7
02:30:49.45 +19:31:49.0
02:27:59.79 +18:29:42.7
02:54:48.92 +23:33:35.0
02:53:16.08 +23:07:39.0
02:27:13.03 +18:34:05.4
02:29:13.86 +19:27:59.3
02:51:12.57 +21:49:55.4
02:55:06.42 +22:49:48.3
02:48:36.57 +19:31:40.9
02:54:30.94 +23:08:45.4
02:55:34.49 +22:04:48.9
02:28:33.47 +18:46:22.6
02:30:28.63 +19:37:44.4
02:33:02.59 +21:37:56.6
02:49:52.83 +20:58:13.7
02:28:30.72 +18:15:36.8
02:31:48.31 +20:53:33.4
02:28:31.84 +19:33:46.3
02:30:21.31 +20:14:14.3
02:53:40.58 +22:49:15.5
02:52:15.94 +21:57:30.0
02:59:38.51 +23:05:13.2
02:56:19.34 +23:20:15.6
02:30:08.58 +20:04:49.8
02:29:14.53 +19:32:29.3
02:29:42.97 +18:46:27.0
02:30:21.06 +18:44:38.5
02:56:09.44 +22:24:59.0
02:31:15.18 +19:53:45.4
02:29:41.93 +20:05:42.6
02:51:56.11 +20:24:47.8
02:27:25.58 +18:07:17.2
02:48:43.22 +20:12:41.1
02:28:28.65 +18:56:39.4
02:27:24.52 +18:15:11.2
02:53:05.73 +22:57:22.4
03:03:41.47 +24:55:39.4
02:50:21.82 +22:30:29.6
02:32:22.04 +18:29:35.3
02:28:50.02 +19:14:10.1
02:56:19.03 +23:32:13.3
02:50:18.15 +21:55:47.4
03:00:42.75 +23:23:52.6
02:55:42.50 +22:27:25.2
02:29:46.13 +20:07:50.1
02:29:02.28 +20:00:35.7
02:31:20.06 +18:40:07.5
02:52:18.73 +22:57:00.0
02:56:37.30 +23:21:34.6
03:05:01.43 +24:56:46.5
03:04:13.32 +24:22:02.2
02:29:46.30 +20:01:14.7
02:31:53.76 +18:26:16.9
02:31:16.30 +19:55:45.8
02:58:18.32 +22:31:40.7
02:31:26.15 +19:16:05.3
02:50:01.35 +20:47:09.6
03:04:46.11 +25:12:30.3
03:02:49.20 +24:37:31.6
02:29:01.86 +19:56:30.6
02:30:30.19 +21:14:03.8
02:31:01.93 +18:43:33.7
02:49:24.89 +20:11:35.0
03:01:53.91 +24:08:51.3
02:28:40.63 +18:49:53.8
02:27:13.42 +18:36:47.5
02:27:49.85 +18:34:08.4
02:50:46.33 +20:53:17.1
02:31:17.58 +18:57:25.4
02:31:59.23 +21:20:47.7
02:28:22.95 +19:07:52.9
02:33:19.66 +21:35:48.2
02:55:07.53 +23:04:39.9
03:04:26.67 +25:44:22.2
03:04:39.28 +25:05:11.8
02:31:16.94 +18:49:19.8
02:49:58.79 +21:37:05.7
03:00:15.12 +23:42:20.9
02:51:26.18 +22:25:55.8
02:55:45.89 +23:03:50.2
02:31:14.76 +18:39:37.6
03:04:40.66 +24:47:38.0
02:55:13.20 +22:39:57.3
02:51:09.05 +20:14:24.3
02:56:39.79 +21:10:15.9
02:52:05.18 +22:04:50.4
02:49:47.56 +20:19:44.2
02:56:00.99 +22:18:26.3
02:50:28.37 +21:22:38.5
02:29:12.20 +19:08:51.9
02:28:54.16 +18:26:47.5
03:02:54.79 +24:52:46.9
02:56:09.10 +23:04:32.7
###################################################################################
02:53:08.81 +20:33:20.9 -- not an asteroid (will add it to exclusion list)
02:33:16.64 +20:21:30.8 -- not an asteroid (will add it to exclusion list)
02:27:17.40 +17:58:32.1 -- not an asteroid (will add it to exclusion list)
02:29:19.15 +18:04:19.3 -- not an asteroid (will add it to exclusion list)
02:29:32.89 +18:19:41.3 -- not an asteroid (will add it to exclusion list)
02:54:35.44 +21:57:40.9 -- not an asteroid (will add it to exclusion list)
02:53:58.97 +21:58:59.1 -- not an asteroid (will add it to exclusion list)
02:30:18.69 +20:52:04.5 -- not an asteroid (will add it to exclusion list)
03:01:56.83 +23:38:27.8 -- not an asteroid (will add it to exclusion list)
03:02:43.08 +25:02:52.9 -- not an asteroid (will add it to exclusion list)
02:27:10.58 +18:39:04.0 -- not an asteroid (will add it to exclusion list)
02:29:29.77 +18:16:03.7 -- not an asteroid (will add it to exclusion list)
02:30:09.00 +19:35:17.0 -- not an asteroid (will add it to exclusion list)
02:52:53.95 +21:07:47.7 -- not an asteroid (will add it to exclusion list)
02:28:32.10 +19:13:01.7 -- not an asteroid (will add it to exclusion list)
02:56:01.46 +22:19:39.0 -- not an asteroid (will add it to exclusion list)
02:46:40.96 +19:00:22.4 -- not an asteroid (will add it to exclusion list)
02:29:42.46 +19:09:36.5 -- not an asteroid (will add it to exclusion list)
02:57:06.80 +23:28:44.5 -- not an asteroid (will add it to exclusion list)
02:52:27.12 +20:26:14.0 -- not an asteroid (will add it to exclusion list)
02:59:34.37 +23:23:01.8 -- not an asteroid (will add it to exclusion list)
02:51:04.00 +21:46:00.8 -- not an asteroid (will add it to exclusion list)
02:31:36.12 +18:58:03.3 -- not an asteroid (will add it to exclusion list)
02:29:46.21 +18:33:54.1 -- not an asteroid (will add it to exclusion list)
02:28:14.10 +18:32:32.1 -- not an asteroid (will add it to exclusion list)
02:28:52.26 +17:59:57.8 -- not an asteroid (will add it to exclusion list)
02:28:24.87 +18:57:20.1 -- not an asteroid (will add it to exclusion list)
02:57:37.01 +22:52:55.8 -- not an asteroid (will add it to exclusion list)
02:50:36.37 +21:14:36.0 -- not an asteroid (will add it to exclusion list)
02:56:17.79 +22:24:50.6 -- not an asteroid (will add it to exclusion list)
02:30:08.49 +19:34:38.8 -- not an asteroid (will add it to exclusion list)
02:28:08.42 +17:47:32.8 -- not an asteroid (will add it to exclusion list)
02:27:25.21 +18:05:46.8 -- not an asteroid (will add it to exclusion list)
02:49:40.89 +20:51:37.7 -- not an asteroid (will add it to exclusion list)
02:48:45.83 +20:45:32.2 -- not an asteroid (will add it to exclusion list)
02:57:12.48 +23:33:18.8 -- not an asteroid (will add it to exclusion list)
03:02:00.60 +23:46:00.2 -- not an asteroid (will add it to exclusion list)
02:53:35.23 +22:27:31.7 -- not an asteroid (will add it to exclusion list)
02:30:49.45 +19:31:49.0 -- not an asteroid (will add it to exclusion list)
02:27:59.79 +18:29:42.7 -- not an asteroid (will add it to exclusion list)
02:54:48.92 +23:33:35.0 -- asteroid (will NOT add it to exclusion list)
02:53:16.08 +23:07:39.0 -- not an asteroid (will add it to exclusion list)
02:27:13.03 +18:34:05.4 -- not an asteroid (will add it to exclusion list)
02:29:13.86 +19:27:59.3 -- not an asteroid (will add it to exclusion list)
02:51:12.57 +21:49:55.4 -- not an asteroid (will add it to exclusion list)
02:55:06.42 +22:49:48.3 -- not an asteroid (will add it to exclusion list)
02:48:36.57 +19:31:40.9 -- not an asteroid (will add it to exclusion list)
02:54:30.94 +23:08:45.4 -- not an asteroid (will add it to exclusion list)
02:55:34.49 +22:04:48.9 -- not an asteroid (will add it to exclusion list)
02:28:33.47 +18:46:22.6 -- not an asteroid (will add it to exclusion list)
02:30:28.63 +19:37:44.4 -- not an asteroid (will add it to exclusion list)
02:33:02.59 +21:37:56.6 -- not an asteroid (will add it to exclusion list)
02:49:52.83 +20:58:13.7 -- not an asteroid (will add it to exclusion list)
02:28:30.72 +18:15:36.8 -- not an asteroid (will add it to exclusion list)
02:31:48.31 +20:53:33.4 -- not an asteroid (will add it to exclusion list)
02:28:31.84 +19:33:46.3 -- not an asteroid (will add it to exclusion list)
02:30:21.31 +20:14:14.3 -- not an asteroid (will add it to exclusion list)
02:53:40.58 +22:49:15.5 -- not an asteroid (will add it to exclusion list)
02:52:15.94 +21:57:30.0 -- not an asteroid (will add it to exclusion list)
02:59:38.51 +23:05:13.2 -- not an asteroid (will add it to exclusion list)
02:56:19.34 +23:20:15.6 -- not an asteroid (will add it to exclusion list)
02:30:08.58 +20:04:49.8 -- not an asteroid (will add it to exclusion list)
02:29:14.53 +19:32:29.3 -- not an asteroid (will add it to exclusion list)
02:29:42.97 +18:46:27.0 -- not an asteroid (will add it to exclusion list)
02:30:21.06 +18:44:38.5 -- not an asteroid (will add it to exclusion list)
02:56:09.44 +22:24:59.0 -- not an asteroid (will add it to exclusion list)
02:31:15.18 +19:53:45.4 -- not an asteroid (will add it to exclusion list)
02:29:41.93 +20:05:42.6 -- not an asteroid (will add it to exclusion list)
02:51:56.11 +20:24:47.8 -- not an asteroid (will add it to exclusion list)
02:27:25.58 +18:07:17.2 -- not an asteroid (will add it to exclusion list)
02:48:43.22 +20:12:41.1 -- not an asteroid (will add it to exclusion list)
02:28:28.65 +18:56:39.4 -- not an asteroid (will add it to exclusion list)
02:27:24.52 +18:15:11.2 -- not an asteroid (will add it to exclusion list)
02:53:05.73 +22:57:22.4 -- not an asteroid (will add it to exclusion list)
03:03:41.47 +24:55:39.4 -- not an asteroid (will add it to exclusion list)
02:50:21.82 +22:30:29.6 -- not an asteroid (will add it to exclusion list)
02:32:22.04 +18:29:35.3 -- not an asteroid (will add it to exclusion list)
02:28:50.02 +19:14:10.1 -- not an asteroid (will add it to exclusion list)
02:56:19.03 +23:32:13.3 -- not an asteroid (will add it to exclusion list)
02:50:18.15 +21:55:47.4 -- not an asteroid (will add it to exclusion list)
03:00:42.75 +23:23:52.6 -- not an asteroid (will add it to exclusion list)
02:55:42.50 +22:27:25.2 -- not an asteroid (will add it to exclusion list)
02:29:46.13 +20:07:50.1 -- not an asteroid (will add it to exclusion list)
02:29:02.28 +20:00:35.7 -- not an asteroid (will add it to exclusion list)
02:31:20.06 +18:40:07.5 -- not an asteroid (will add it to exclusion list)
02:52:18.73 +22:57:00.0 -- not an asteroid (will add it to exclusion list)
02:56:37.30 +23:21:34.6 -- not an asteroid (will add it to exclusion list)
03:05:01.43 +24:56:46.5 -- not an asteroid (will add it to exclusion list)
03:04:13.32 +24:22:02.2 -- not an asteroid (will add it to exclusion list)
02:29:46.30 +20:01:14.7 -- not an asteroid (will add it to exclusion list)
02:31:53.76 +18:26:16.9 -- not an asteroid (will add it to exclusion list)
02:31:16.30 +19:55:45.8 -- not an asteroid (will add it to exclusion list)
02:58:18.32 +22:31:40.7 -- not an asteroid (will add it to exclusion list)
02:31:26.15 +19:16:05.3 -- not an asteroid (will add it to exclusion list)
02:50:01.35 +20:47:09.6 -- not an asteroid (will add it to exclusion list)
03:04:46.11 +25:12:30.3 -- not an asteroid (will add it to exclusion list)
03:02:49.20 +24:37:31.6 -- not an asteroid (will add it to exclusion list)
02:29:01.86 +19:56:30.6 -- not an asteroid (will add it to exclusion list)
02:30:30.19 +21:14:03.8 -- not an asteroid (will add it to exclusion list)
02:31:01.93 +18:43:33.7 -- not an asteroid (will add it to exclusion list)
02:49:24.89 +20:11:35.0 -- not an asteroid (will add it to exclusion list)
03:01:53.91 +24:08:51.3 -- not an asteroid (will add it to exclusion list)
02:28:40.63 +18:49:53.8 -- not an asteroid (will add it to exclusion list)
02:27:13.42 +18:36:47.5 -- not an asteroid (will add it to exclusion list)
02:27:49.85 +18:34:08.4 -- not an asteroid (will add it to exclusion list)
02:50:46.33 +20:53:17.1 -- not an asteroid (will add it to exclusion list)
02:31:17.58 +18:57:25.4 -- not an asteroid (will add it to exclusion list)
02:31:59.23 +21:20:47.7 -- not an asteroid (will add it to exclusion list)
02:28:22.95 +19:07:52.9 -- not an asteroid (will add it to exclusion list)
02:33:19.66 +21:35:48.2 -- not an asteroid (will add it to exclusion list)
02:55:07.53 +23:04:39.9 -- not an asteroid (will add it to exclusion list)
03:04:26.67 +25:44:22.2 -- not an asteroid (will add it to exclusion list)
03:04:39.28 +25:05:11.8 -- not an asteroid (will add it to exclusion list)
02:31:16.94 +18:49:19.8 -- not an asteroid (will add it to exclusion list)
02:49:58.79 +21:37:05.7 -- not an asteroid (will add it to exclusion list)
03:00:15.12 +23:42:20.9 -- not an asteroid (will add it to exclusion list)
02:51:26.18 +22:25:55.8 -- not an asteroid (will add it to exclusion list)
02:55:45.89 +23:03:50.2 -- not an asteroid (will add it to exclusion list)
02:31:14.76 +18:39:37.6 -- not an asteroid (will add it to exclusion list)
03:04:40.66 +24:47:38.0 -- not an asteroid (will add it to exclusion list)
02:55:13.20 +22:39:57.3 -- not an asteroid (will add it to exclusion list)
02:51:09.05 +20:14:24.3 -- not an asteroid (will add it to exclusion list)
02:56:39.79 +21:10:15.9 -- not an asteroid (will add it to exclusion list)
02:52:05.18 +22:04:50.4 -- not an asteroid (will add it to exclusion list)
02:49:47.56 +20:19:44.2 -- not an asteroid (will add it to exclusion list)
02:56:00.99 +22:18:26.3 -- not an asteroid (will add it to exclusion list)
02:50:28.37 +21:22:38.5 -- not an asteroid (will add it to exclusion list)
02:29:12.20 +19:08:51.9 -- not an asteroid (will add it to exclusion list)
02:28:54.16 +18:26:47.5 -- not an asteroid (will add it to exclusion list)
03:02:54.79 +24:52:46.9 -- not an asteroid (will add it to exclusion list)
02:56:09.10 +23:04:32.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
02:27:10.58 +18:39:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:13.03 +18:34:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:13.42 +18:36:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:17.40 +17:58:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:24.52 +18:15:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:25.21 +18:05:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:25.58 +18:07:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:49.85 +18:34:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:59.79 +18:29:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:08.42 +17:47:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:14.10 +18:32:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:22.95 +19:07:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:24.87 +18:57:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:28.65 +18:56:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:30.72 +18:15:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:31.84 +19:33:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:32.10 +19:13:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:33.47 +18:46:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:40.63 +18:49:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:50.02 +19:14:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:52.26 +17:59:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:54.16 +18:26:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:01.86 +19:56:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:02.28 +20:00:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:12.20 +19:08:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:13.86 +19:27:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:14.53 +19:32:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:19.15 +18:04:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:29.77 +18:16:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:32.89 +18:19:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:41.93 +20:05:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:42.46 +19:09:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:42.97 +18:46:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:46.13 +20:07:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:46.21 +18:33:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:46.30 +20:01:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:08.49 +19:34:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:08.58 +20:04:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:09.00 +19:35:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:18.69 +20:52:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:21.06 +18:44:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:21.31 +20:14:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:28.63 +19:37:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:30.19 +21:14:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:49.45 +19:31:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:01.93 +18:43:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:14.76 +18:39:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:15.18 +19:53:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:16.30 +19:55:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:16.94 +18:49:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:17.58 +18:57:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:20.06 +18:40:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:26.15 +19:16:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:36.12 +18:58:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:48.31 +20:53:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:53.76 +18:26:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:59.23 +21:20:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:22.04 +18:29:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:02.59 +21:37:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:16.64 +20:21:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:19.66 +21:35:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:46:40.96 +19:00:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:36.57 +19:31:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:43.22 +20:12:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:45.83 +20:45:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:24.89 +20:11:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:40.89 +20:51:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:47.56 +20:19:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:52.83 +20:58:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:58.79 +21:37:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:01.35 +20:47:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:18.15 +21:55:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:21.82 +22:30:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:28.37 +21:22:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:36.37 +21:14:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:46.33 +20:53:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:04.00 +21:46:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:09.05 +20:14:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:12.57 +21:49:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:26.18 +22:25:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:56.11 +20:24:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:05.18 +22:04:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:15.94 +21:57:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:18.73 +22:57:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:27.12 +20:26:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:53.95 +21:07:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:05.73 +22:57:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:08.81 +20:33:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:16.08 +23:07:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:35.23 +22:27:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:40.58 +22:49:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:58.97 +21:58:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:30.94 +23:08:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:35.44 +21:57:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:06.42 +22:49:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:07.53 +23:04:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:13.20 +22:39:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:34.49 +22:04:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:42.50 +22:27:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:45.89 +23:03:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:00.99 +22:18:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:01.46 +22:19:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:09.10 +23:04:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:09.44 +22:24:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:17.79 +22:24:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:19.03 +23:32:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:19.34 +23:20:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:37.30 +23:21:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:39.79 +21:10:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:06.80 +23:28:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:12.48 +23:33:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:37.01 +22:52:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:18.32 +22:31:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:34.37 +23:23:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:38.51 +23:05:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:15.12 +23:42:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:42.75 +23:23:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:53.91 +24:08:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:56.83 +23:38:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:00.60 +23:46:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:43.08 +25:02:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:49.20 +24:37:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:54.79 +24:52:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:41.47 +24:55:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:13.32 +24:22:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:26.67 +25:44:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:39.28 +25:05:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:40.66 +24:47:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:46.11 +25:12:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:01.43 +24:56:46.5 -- 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)
02:27:10.58 +18:39:04.0 -- not a known variable star
02:27:13.03 +18:34:05.4 -- not a known variable star
02:27:13.42 +18:36:47.5 -- not a known variable star
02:27:17.40 +17:58:32.1 -- not a known variable star
02:27:24.52 +18:15:11.2 -- not a known variable star
02:27:25.21 +18:05:46.8 -- not a known variable star
02:27:25.58 +18:07:17.2 -- not a known variable star
02:27:49.85 +18:34:08.4 -- not a known variable star
02:27:59.79 +18:29:42.7 -- not a known variable star
02:28:08.42 +17:47:32.8 -- not a known variable star
02:28:14.10 +18:32:32.1 -- not a known variable star
02:28:22.95 +19:07:52.9 -- not a known variable star
02:28:24.87 +18:57:20.1 -- not a known variable star
02:28:28.65 +18:56:39.4 -- not a known variable star
02:28:30.72 +18:15:36.8 -- not a known variable star
02:28:31.84 +19:33:46.3 -- not a known variable star
02:28:32.10 +19:13:01.7 -- not a known variable star
02:28:33.47 +18:46:22.6 -- not a known variable star
02:28:40.63 +18:49:53.8 -- not a known variable star
02:28:50.02 +19:14:10.1 -- not a known variable star
02:28:52.26 +17:59:57.8 -- not a known variable star
02:28:54.16 +18:26:47.5 -- not a known variable star
02:29:01.86 +19:56:30.6 -- not a known variable star
02:29:02.28 +20:00:35.7 -- not a known variable star
02:29:12.20 +19:08:51.9 -- not a known variable star
02:29:13.86 +19:27:59.3 -- not a known variable star
02:29:14.53 +19:32:29.3 -- not a known variable star
02:29:19.15 +18:04:19.3 -- not a known variable star
02:29:29.77 +18:16:03.7 -- not a known variable star
02:29:32.89 +18:19:41.3 -- not a known variable star
02:29:41.93 +20:05:42.6 -- not a known variable star
02:29:42.46 +19:09:36.5 -- not a known variable star
02:29:42.97 +18:46:27.0 -- not a known variable star
02:29:46.13 +20:07:50.1 -- not a known variable star
02:29:46.21 +18:33:54.1 -- not a known variable star
02:29:46.30 +20:01:14.7 -- not a known variable star
02:30:08.49 +19:34:38.8 -- not a known variable star
02:30:08.58 +20:04:49.8 -- not a known variable star
02:30:09.00 +19:35:17.0 -- not a known variable star
02:30:18.69 +20:52:04.5 -- not a known variable star
02:30:21.06 +18:44:38.5 -- not a known variable star
02:30:21.31 +20:14:14.3 -- not a known variable star
02:30:28.63 +19:37:44.4 -- not a known variable star
02:30:30.19 +21:14:03.8 -- not a known variable star
02:30:49.45 +19:31:49.0 -- not a known variable star
02:31:01.93 +18:43:33.7 -- not a known variable star
02:31:14.76 +18:39:37.6 -- not a known variable star
02:31:15.18 +19:53:45.4 -- not a known variable star
02:31:16.30 +19:55:45.8 -- not a known variable star
02:31:16.94 +18:49:19.8 -- not a known variable star
02:31:17.58 +18:57:25.4 -- not a known variable star
02:31:20.06 +18:40:07.5 -- not a known variable star
02:31:26.15 +19:16:05.3 -- not a known variable star
02:31:36.12 +18:58:03.3 -- not a known variable star
02:31:48.31 +20:53:33.4 -- not a known variable star
02:31:53.76 +18:26:16.9 -- not a known variable star
02:31:59.23 +21:20:47.7 -- not a known variable star
02:32:22.04 +18:29:35.3 -- not a known variable star
02:33:02.59 +21:37:56.6 -- not a known variable star
02:33:16.64 +20:21:30.8 -- not a known variable star
02:33:19.66 +21:35:48.2 -- not a known variable star
02:46:40.96 +19:00:22.4 -- not a known variable star
02:48:36.57 +19:31:40.9 -- not a known variable star
02:48:43.22 +20:12:41.1 -- a known variable star
02:48:45.83 +20:45:32.2 -- not a known variable star
02:49:24.89 +20:11:35.0 -- not a known variable star
02:49:40.89 +20:51:37.7 -- not a known variable star
02:49:47.56 +20:19:44.2 -- not a known variable star
02:49:52.83 +20:58:13.7 -- not a known variable star
02:49:58.79 +21:37:05.7 -- not a known variable star
02:50:01.35 +20:47:09.6 -- not a known variable star
02:50:18.15 +21:55:47.4 -- not a known variable star
02:50:21.82 +22:30:29.6 -- not a known variable star
02:50:28.37 +21:22:38.5 -- not a known variable star
02:50:36.37 +21:14:36.0 -- not a known variable star
02:50:46.33 +20:53:17.1 -- not a known variable star
02:51:04.00 +21:46:00.8 -- not a known variable star
02:51:09.05 +20:14:24.3 -- a known variable star
02:51:12.57 +21:49:55.4 -- not a known variable star
02:51:26.18 +22:25:55.8 -- not a known variable star
02:51:56.11 +20:24:47.8 -- not a known variable star
02:52:05.18 +22:04:50.4 -- not a known variable star
02:52:15.94 +21:57:30.0 -- not a known variable star
02:52:18.73 +22:57:00.0 -- not a known variable star
02:52:27.12 +20:26:14.0 -- not a known variable star
02:52:53.95 +21:07:47.7 -- not a known variable star
02:53:05.73 +22:57:22.4 -- a known variable star
02:53:08.81 +20:33:20.9 -- not a known variable star
02:53:16.08 +23:07:39.0 -- not a known variable star
02:53:35.23 +22:27:31.7 -- not a known variable star
02:53:40.58 +22:49:15.5 -- not a known variable star
02:53:58.97 +21:58:59.1 -- not a known variable star
02:54:30.94 +23:08:45.4 -- not a known variable star
02:54:35.44 +21:57:40.9 -- not a known variable star
02:55:06.42 +22:49:48.3 -- not a known variable star
02:55:07.53 +23:04:39.9 -- not a known variable star
02:55:13.20 +22:39:57.3 -- not a known variable star
02:55:34.49 +22:04:48.9 -- not a known variable star
02:55:42.50 +22:27:25.2 -- not a known variable star
02:55:45.89 +23:03:50.2 -- not a known variable star
02:56:00.99 +22:18:26.3 -- not a known variable star
02:56:01.46 +22:19:39.0 -- not a known variable star
02:56:09.10 +23:04:32.7 -- not a known variable star
02:56:09.44 +22:24:59.0 -- not a known variable star
02:56:17.79 +22:24:50.6 -- not a known variable star
02:56:19.03 +23:32:13.3 -- a known variable star
02:56:19.34 +23:20:15.6 -- not a known variable star
02:56:37.30 +23:21:34.6 -- not a known variable star
02:56:39.79 +21:10:15.9 -- not a known variable star
02:57:06.80 +23:28:44.5 -- not a known variable star
02:57:12.48 +23:33:18.8 -- not a known variable star
02:57:37.01 +22:52:55.8 -- not a known variable star
02:58:18.32 +22:31:40.7 -- not a known variable star
02:59:34.37 +23:23:01.8 -- not a known variable star
02:59:38.51 +23:05:13.2 -- a known variable star
03:00:15.12 +23:42:20.9 -- not a known variable star
03:00:42.75 +23:23:52.6 -- not a known variable star
03:01:53.91 +24:08:51.3 -- a known variable star
03:01:56.83 +23:38:27.8 -- not a known variable star
03:02:00.60 +23:46:00.2 -- a known variable star
03:02:43.08 +25:02:52.9 -- not a known variable star
03:02:49.20 +24:37:31.6 -- a known variable star
03:02:54.79 +24:52:46.9 -- not a known variable star
03:03:41.47 +24:55:39.4 -- not a known variable star
03:04:13.32 +24:22:02.2 -- not a known variable star
03:04:26.67 +25:44:22.2 -- not a known variable star
03:04:39.28 +25:05:11.8 -- not a known variable star
03:04:40.66 +24:47:38.0 -- not a known variable star
03:04:46.11 +25:12:30.3 -- not a known variable star
03:05:01.43 +24:56:46.5 -- not a known variable star
Found 122 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
130 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 130 (excluding asteroids and hot pixels, 122 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)2461231.87639127 -observatory V36
07:32:12.76 +17:07:57.7 Mercury (5.1mag)
10:11:45.35 +12:40:19.0 Venus (-4.1mag)
04:24:14.94 +21:25:24.1 Mars (1.3mag)
08:16:41.98 +20:11:24.6 Jupiter (-1.8mag)
00:55:51.08 +03:20:29.5 Saturn (0.7mag)
04:07:14.34 +20:45:04.2 Uranus (5.8mag)
00:17:01.49 +00:20:41.1 Neptune (7.8mag)
20:30:54.80 -23:18:01.3 Pluto (14.4mag)
03:13:21.28 +22:30:16.8 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 05:53 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.87639127:
08:16:49.00 +20:11:00.0 Io (6.1mag)
08:16:45.29 +20:11:14.1 Europa (6.3mag)
08:16:59.15 +20:10:22.4 Ganymede (5.6mag)
08:17:09.85 +20:09:41.5 Callisto (6.8mag)
08:15:13.40 +19:55:34.8 Himalia (15.7mag)
08:16:41.92 +20:11:25.6 Thebe (16.6mag)
08:14:34.73 +20:00:04.0 Elara (17.6mag)
08:20:14.25 +20:05:33.9 Pasiphae (17.8mag)
08:21:39.74 +20:16:29.8 Carme (19.0mag)
00:55:41.00 +03:20:20.0 Titan (8.5mag)
00:55:45.83 +03:20:32.0 Rhea (9.8mag)
00:55:20.34 +03:19:38.0 Iapetus (11.2mag)
00:56:00.22 +03:20:48.7 Hyperion (14.5mag)
00:55:51.77 +03:17:43.0 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 05:54 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.87639127:
17:46:03.57 -32:58:14.2 JWST
16:18:39.79 +47:54:47.9 Chandra
04:30:32.61 +53:04:02.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 05:53 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.87639127 -observatory V36
02:36:18.30 +14:25:52.6 17.9mag P/1996 R2 (Lagerkvist)
18:17:55.19 -34:21:47.9 13.7mag P/2010 H2 (Vales)
06:25:41.98 -68:08:24.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:48.90 +32:26:50.6 17.6mag C/2017 K2 (PANSTARRS)
17:03:06.52 +16:02:54.0 18.0mag C/2021 G2 (ATLAS)
01:47:56.84 +08:16:16.7 15.4mag P/2021 N1 (ZTF)
22:59:30.99 +32:17:08.1 17.3mag C/2022 E2 (ATLAS)
06:12:25.69 +26:55:34.0 16.7mag C/2022 N2 (PANSTARRS)
09:55:32.21 +29:46:47.2 16.8mag C/2022 QE78 (ATLAS)
09:09:45.08 +04:59:58.9 17.8mag C/2022 R6 (PANSTARRS)
18:07:12.16 +21:17:34.6 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.07 -11:23:17.9 17.7mag P/2023 B1 (PANSTARRS)
21:49:12.28 +67:37:16.4 17.8mag C/2023 H5 (Lemmon)
16:30:50.16 -10:04:50.8 13.9mag C/2023 R1 (PANSTARRS)
08:00:41.62 +65:42:35.1 17.9mag C/2024 A1 (ATLAS)
07:32:50.84 +30:00:16.7 14.6mag C/2024 E1 (Wierzchos)
15:16:18.84 +15:19:44.5 17.5mag C/2024 G6 (ATLAS)
19:41:16.68 +39:23:52.6 13.8mag C/2024 J3 (ATLAS)
21:47:33.44 +46:00:25.3 17.8mag C/2024 R4 (PANSTARRS)
04:49:39.76 -13:47:41.2 15.7mag C/2024 T5 (ATLAS)
06:34:35.64 +29:03:56.9 18.0mag C/2025 J1 (Borisov)
07:14:21.44 -12:53:30.5 16.5mag C/2025 R3 (PANSTARRS)
09:56:07.22 +22:26:08.9 17.6mag C/2025 V2 (Rankin)
12:44:37.51 +03:56:12.4 17.1mag C/2025 Y1 (ATLAS)
16:51:52.92 +79:07:14.9 17.4mag C/2026 A2 (Bok)
02:46:18.14 +45:14:27.6 16.7mag C/2026 B2 (Sun-Gao)
11:25:31.62 +04:32:54.8 16.9mag A/2026 E1
21:19:04.33 -15:05:06.0 7.3mag 10P/Tempel
11:13:27.99 -01:53:17.6 16.1mag 29P/Schwassmann-Wachmann
04:00:12.45 +29:33:21.2 17.8mag 47P/Ashbrook-Jackson
10:08:07.67 +14:00:13.3 17.0mag 63P/Wild
00:48:22.38 -05:05:34.2 15.5mag 65P/Gunn
08:27:01.77 +34:13:03.8 17.9mag 76P/West-Kohoutek-Ikemura
04:27:27.42 +20:10:48.5 13.7mag 78P/Gehrels
02:22:22.43 +10:36:46.6 16.2mag 88P/Howell
06:35:36.20 +30:32:00.5 15.7mag 93P/Lovas
04:21:04.67 +31:07:27.1 16.9mag 114P/Wiseman-Skiff
08:08:45.24 +30:42:03.2 15.2mag 123P/West-Hartley
10:48:10.61 +01:10:37.4 16.8mag 124P/Mrkos
04:51:46.04 +20:48:49.4 16.2mag 128P/Shoemaker-Holt
05:36:18.09 +19:42:50.1 17.8mag 131P/Mueller
00:01:33.12 +02:56:10.4 17.9mag 139P/Vaisala-Oterma
07:13:39.15 +17:00:56.1 15.5mag 141P-D/Machholz
03:16:51.58 -21:06:14.1 15.5mag 161P/Hartley-IRAS
05:33:09.05 +33:57:14.5 15.3mag 162P/SidingSpring
19:04:24.63 +15:05:49.0 14.7mag 169P/NEAT
01:41:05.27 +07:36:05.3 17.7mag 220P/McNaught
16:35:57.88 -08:23:10.5 17.0mag 235P/LINEAR
08:45:20.22 +33:17:50.1 17.9mag 240P/NEAT
20:42:09.77 -49:34:33.7 17.8mag 259P/Garradd
01:59:22.41 +12:06:22.0 15.7mag 260P/McNaught
05:37:17.97 +36:50:42.0 17.4mag 295P/LINEAR
15:06:36.70 +06:03:17.2 17.6mag 391P/Kowalski
08:34:37.52 +19:40:32.9 17.9mag 450P/LONEOS
07:51:48.29 +39:12:51.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 05:54 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 10 05:53 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 05:53 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 05:53 tns_transients_list.txt
