This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7
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 15.1591 2461236.6591 12.52 23:34:30.37 +54:23:52.2
111.79662 -6.80219 galactic Cas Second-epoch detections are separated by 4.0" 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 | target | 23:34:30.37 +54:23:52.2 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.041 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:30.37 +54:23:52.2: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:30.37 +54:23:52.2: 13.30 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 34 30.37 +54 23 52.2 12.5 U Cas 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,2461236.6591,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.19 23:37:25.08 +51:16:42.3
111.30447 -9.91455 galactic Cas Second-epoch detections are separated by 1.5" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J354.3430+51.2841 | 23:37:22.48 +51:16:29.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:25.08 +51:16:42.3: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:25.08 +51:16:42.3: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 37 25.08 +51 16 42.3 12.2 U Cas 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 J354.3430+51.2841,2461236.6591,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.3430+51.2841 20260715.1591 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.32 23:37:44.91 +53:08:11.5
111.89061 -8.14818 galactic Cas Second-epoch detections are separated by 2.5" 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 | 23:37:44.91 +53:08:11.5 (user input) | T | P | (position from user input) J-Ks=1.037+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:44.91 +53:08:11.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:44.91 +53:08:11.5: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 37 44.91 +53 08 11.5 12.3 U Cas 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,2461236.6591,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.37 23:26:13.25 +57:06:48.2
111.52804 -3.85952 galactic Cas Second-epoch detections are separated by 0.9" and 10.2 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 J351.5671+57.1154 | 23:26:13.25 +57:06:48.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.924+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:13.25 +57:06:48.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:13.25 +57:06:48.2: 13.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 26 13.25 +57 06 48.2 12.4 U Cas 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 J351.5671+57.1154,2461236.6591,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.5671+57.1154 20260715.1591 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.12 23:44:33.09 +53:02:41.9
112.85896 -8.51364 galactic Cas Second-epoch detections are separated by 2.9" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:33.09 +53:02:41.9 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:33.09 +53:02:41.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:33.09 +53:02:41.9: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 44 33.09 +53 02 41.9 12.1 U Cas 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,2461236.6591,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.06 23:42:49.01 +51:38:40.2
112.22744 -9.79536 galactic Cas Second-epoch detections are separated by 4.4" and 9.8 pix
The object was found in VSX12" Gaia DR3 1944698729926124800
Type: ROT
# Max. Min./Amp. JD0 Period
16.800 G 16.860 G K
ATTENTION: measured mag 12.06 is 4.7 mag brighter than the VSX record maximum brightness 16.80 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:49.01 +51:38:40.2: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:49.01 +51:38:40.2: 13.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 42 49.01 +51 38 40.2 12.1 U Cas 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 1944698729926124800,2461236.6591,12.06,0.05,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
Gaia DR3 1944698729926124800 20260715.1591 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 15.1591 2461236.6591 12.32 23:26:09.41 +56:23:37.1
111.28565 -4.53751 galactic Cas Second-epoch detections are separated by 0.3" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:09.41 +56:23:37.1 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:09.41 +56:23:37.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:09.41 +56:23:37.1: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 26 09.41 +56 23 37.1 12.3 U Cas 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,2461236.6591,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.48 23:20:07.64 +54:31:56.6
109.84949 -6.00347 galactic Cas Second-epoch detections are separated by 0.7" and 10.2 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 1996047670988256896 | 23:20:05.64 +54:31:39.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.815+/-0.027 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:07.64 +54:31:56.6: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:07.64 +54:31:56.6: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 20 07.64 +54 31 56.6 12.5 U Cas 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 1996047670988256896,2461236.6591,12.48,0.05,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 1996047670988256896 20260715.1591 12.48CV 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 15.1591 2461236.6591 12.29 23:19:22.11 +53:12:39.3
109.27974 -7.20284 galactic Cas Second-epoch detections are separated by 0.6" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:19:22.11 +53:12:39.3 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:22.11 +53:12:39.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:22.11 +53:12:39.3: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 19 22.11 +53 12 39.3 12.3 U Cas 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,2461236.6591,12.29,0.05,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
target 20260715.1591 12.29CV 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 15.1591 2461236.6591 12.17 23:28:30.28 +52:00:34.9
110.19331 -8.79896 galactic Cas Second-epoch detections are separated by 0.2" and 10.3 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 1991633857658147712 | 23:28:30.85 +51:59:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.293+/- (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:30.28 +52:00:34.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:30.28 +52:00:34.9: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 28 30.28 +52 00 34.9 12.2 U Cas 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 1991633857658147712,2461236.6591,12.17,0.05,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 1991633857658147712 20260715.1591 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.23 23:34:59.88 +56:37:34.9
112.52152 -4.69244 galactic Cas Second-epoch detections are separated by 1.4" 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 | 23:34:59.88 +56:37:34.9 (user input) | T | P | (position from user input) J-Ks=0.294+/-0.037 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:59.88 +56:37:34.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:59.88 +56:37:34.9: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 34 59.88 +56 37 34.9 12.2 U Cas 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,2461236.6591,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.13 23:43:59.07 +55:38:49.6
113.45851 -5.97903 galactic Cas Second-epoch detections are separated by 0.7" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:43:59.07 +55:38:49.6 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:59.07 +55:38:49.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:59.07 +55:38:49.6: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 43 59.07 +55 38 49.6 12.1 U Cas 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,2461236.6591,12.13,0.05,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 20260715.1591 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.21 23:21:10.57 +53:55:06.4
109.78080 -6.63257 galactic Cas Second-epoch detections are separated by 1.5" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.2971+53.9128 | 23:21:10.67 +53:55:28.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:10.57 +53:55:06.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:10.57 +53:55:06.4: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 21 10.57 +53 55 06.4 12.2 U Cas 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 J350.2971+53.9128,2461236.6591,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.2971+53.9128 20260715.1591 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.23 23:14:45.63 +54:00:29.4
108.92526 -6.21353 galactic Cas Second-epoch detections are separated by 1.1" and 10.5 pix
The object was found in VSX 3" ZTF J231445.46+540031.4
Type: RS
# Max. Min./Amp. JD0 Period
14.072 r Y 0.060 r 2458355.94040 0.442172600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:45.63 +54:00:29.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:45.63 +54:00:29.4: 13.31 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 14 45.63 +54 00 29.4 12.2 U Cas 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
ZTF J231445.46+540031.4,2461236.6591,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231445.46+540031.4 20260715.1591 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.99 23:43:23.53 +57:27:47.9
113.85407 -4.20421 galactic Cas Second-epoch detections are separated by 1.9" and 10.0 pix
The object was found in VSX 2" Gaia DR3 1998661386231043584
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:23.53 +57:27:47.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:23.53 +57:27:47.9: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 43 23.53 +57 27 47.9 12.0 U Cas 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 1998661386231043584,2461236.6591,11.99,0.05,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 1998661386231043584 20260715.1591 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.09 23:41:45.35 +55:45:22.5
113.18299 -5.79096 galactic Cas Second-epoch detections are separated by 0.7" 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 | 23:41:45.35 +55:45:22.5 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:45.35 +55:45:22.5: 13.47 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:45.35 +55:45:22.5: 13.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.47 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 41 45.35 +55 45 22.5 12.1 U Cas 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,2461236.6591,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.11 23:28:04.20 +53:15:53.6
110.53487 -7.58835 galactic Cas Second-epoch detections are separated by 4.5" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.0346+53.2664 | 23:28:07.60 +53:15:23.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:04.20 +53:15:53.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:04.20 +53:15:53.6: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 28 04.20 +53 15 53.6 12.1 U Cas 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 J352.0346+53.2664,2461236.6591,12.11,0.05,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
ATO J352.0346+53.2664 20260715.1591 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 15.1591 2461236.6591 11.93 23:53:29.64 +54:54:32.6
114.60111 -7.02272 galactic Cas Second-epoch detections are separated by 0.0" 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 | 23:53:29.64 +54:54:32.6 (user input) | T | P | (position from user input) J-Ks=0.980+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:29.64 +54:54:32.6: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:29.64 +54:54:32.6: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 53 29.64 +54 54 32.6 11.9 U Cas 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,2461236.6591,11.93,0.05,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 20260715.1591 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 15.1591 2461236.6591 11.88 23:32:25.74 +51:54:36.1
110.74335 -9.08210 galactic Cas Second-epoch detections are separated by 0.9" and 10.3 pix
The object was found in VSX 2" Gaia DR3 1992931384459555584
Type: VAR
# Max. Min./Amp. JD0 Period
13.620 G 13.760 G 0.014758400000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:25.74 +51:54:36.1: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:25.74 +51:54:36.1: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 32 25.74 +51 54 36.1 11.9 U Cas 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 1992931384459555584,2461236.6591,11.88,0.05,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 1992931384459555584 20260715.1591 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 15.1591 2461236.6591 11.87 23:37:50.57 +50:59:28.9
111.28592 -10.20868 galactic Cas Second-epoch detections are separated by 2.1" and 10.4 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 J354.4519+51.0005 | 23:37:48.45 +51:00:02.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.351+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:50.57 +50:59:28.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:50.57 +50:59:28.9: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 37 50.57 +50 59 28.9 11.9 U Cas 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 J354.4519+51.0005,2461236.6591,11.87,0.05,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
ATO J354.4519+51.0005 20260715.1591 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 15.1591 2461236.6591 11.98 23:30:56.77 +51:10:34.7
110.29223 -9.70933 galactic Cas Second-epoch detections are separated by 3.8" 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 | 23:30:56.77 +51:10:34.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:56.77 +51:10:34.7: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:56.77 +51:10:34.7: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 30 56.77 +51 10 34.7 12.0 U Cas 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,2461236.6591,11.98,0.05,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 20260715.1591 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 15.1591 2461236.6591 11.78 23:44:50.48 +50:30:38.3
112.23609 -10.97292 galactic Cas Second-epoch detections are separated by 1.4" and 10.2 pix
The object was found in VSX21" Gaia DR3 1943787062988330752
Type: ROT
# Max. Min./Amp. JD0 Period
16.530 G 16.590 G G
ATTENTION: measured mag 11.78 is 4.8 mag brighter than the VSX record maximum brightness 16.53 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:50.48 +50:30:38.3: 13.53 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:50.48 +50:30:38.3: 13.16 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 44 50.48 +50 30 38.3 11.8 U Cas 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 1943787062988330752,2461236.6591,11.78,0.05,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 1943787062988330752 20260715.1591 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 15.1591 2461236.6591 12.12 23:23:08.06 +57:09:44.1
111.14803 -3.67537 galactic Cas Second-epoch detections are separated by 2.9" and 9.8 pix
The object was found in VSX22" Gaia DR3 2009326472917565952
Type:
# Max. Min./Amp. JD0 Period
13.070 G 13.110 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:08.06 +57:09:44.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:08.06 +57:09:44.1: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 23 08.06 +57 09 44.1 12.1 U Cas 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 2009326472917565952,2461236.6591,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009326472917565952 20260715.1591 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.13 23:23:39.57 +52:23:57.9
109.61315 -8.18766 galactic And Second-epoch detections are separated by 4.7" 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 | 23:23:39.57 +52:23:57.9 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:39.57 +52:23:57.9: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:39.57 +52:23:57.9: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 23 39.57 +52 23 57.9 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461236.6591,12.13,0.05,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 20260715.1591 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.09 23:22:55.66 +54:58:03.6
110.38084 -5.73266 galactic Cas Second-epoch detections are separated by 1.7" and 10.4 pix
The object was found in VSX13" Gaia DR3 1996157145418575488
Type: E
# Max. Min./Amp. JD0 Period
15.990 G 16.060 G 2.162030000000 F
ATTENTION: measured mag 12.09 is 3.9 mag brighter than the VSX record maximum brightness 15.99 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:55.66 +54:58:03.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:55.66 +54:58:03.6: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 22 55.66 +54 58 03.6 12.1 U Cas 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 1996157145418575488,2461236.6591,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996157145418575488 20260715.1591 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.96 00:01:47.84 +56:08:37.0
116.01667 -6.06019 galactic Cas Second-epoch detections are separated by 2.2" and 10.0 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 | 00:01:47.84 +56:08:37.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:47.84 +56:08:37.0: 13.78 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:47.84 +56:08:37.0: 13.18 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 00 01 47.84 +56 08 37.0 12.0 U Cas 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,2461236.6591,11.96,0.05,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 20260715.1591 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 15.1591 2461236.6591 11.62 23:52:21.36 +51:55:18.8
113.74774 -9.89318 galactic Cas Second-epoch detections are separated by 1.8" 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 | 23:52:21.36 +51:55:18.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:21.36 +51:55:18.8: 12.74 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:21.36 +51:55:18.8: 12.52 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 52 21.36 +51 55 18.8 11.6 U Cas 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,2461236.6591,11.62,0.05,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
target 20260715.1591 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 15.1591 2461236.6591 11.97 23:35:20.19 +54:55:23.7
112.06743 -6.33518 galactic Cas Second-epoch detections are separated by 1.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.8332+54.9240 | 23:35:22.33 +54:55:14.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:20.19 +54:55:23.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:20.19 +54:55:23.7: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 35 20.19 +54 55 23.7 12.0 U Cas 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 J353.8332+54.9240,2461236.6591,11.97,0.05,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 J353.8332+54.9240 20260715.1591 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.82 23:54:14.13 +55:25:04.5
114.81924 -6.55024 galactic Cas Second-epoch detections are separated by 0.9" and 9.5 pix
The object was found in VSX17" Gaia DR3 1994685895781406336
Type:
# Max. Min./Amp. JD0 Period
13.010 G 13.050 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:14.13 +55:25:04.5: 12.90 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:14.13 +55:25:04.5: 12.71 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 54 14.13 +55 25 04.5 11.8 U Cas 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 1994685895781406336,2461236.6591,11.82,0.05,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 1994685895781406336 20260715.1591 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 15.1591 2461236.6591 11.90 23:31:48.28 +56:54:17.2
112.18585 -4.29625 galactic Cas Second-epoch detections are separated by 0.3" and 10.0 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 1998596652484201600 | 23:31:48.61 +56:53:39.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:48.28 +56:54:17.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:48.28 +56:54:17.2: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 31 48.28 +56 54 17.2 11.9 U Cas 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 1998596652484201600,2461236.6591,11.90,0.05,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
Gaia DR3 1998596652484201600 20260715.1591 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 15.1591 2461236.6591 11.44 00:24:30.27 +57:44:07.9
119.32995 -4.94773 galactic Cas Second-epoch detections are separated by 1.9" 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 422083031936705536 | 00:24:27.49 +57:43:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:30.27 +57:44:07.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:30.27 +57:44:07.9: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 24 30.27 +57 44 07.9 11.4 U Cas 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 422083031936705536,2461236.6591,11.44,0.05,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 422083031936705536 20260715.1591 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 15.1591 2461236.6591 11.67 23:28:57.53 +51:01:10.4
109.94172 -9.76006 galactic Cas Second-epoch detections are separated by 0.5" and 10.3 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 | 23:28:57.53 +51:01:10.4 (user input) | T | P | (position from user input) J-Ks=0.660+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:57.53 +51:01:10.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:57.53 +51:01:10.4: 13.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 28 57.53 +51 01 10.4 11.7 U Cas 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,2461236.6591,11.67,0.05,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
target 20260715.1591 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 15.1591 2461236.6591 11.72 23:44:50.71 +54:41:18.2
113.32885 -6.93697 galactic Cas Second-epoch detections are separated by 2.2" and 9.8 pix
The object was found in VSX 1" Gaia DR3 1994179536316071424
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.760 G 13.800 G 0.027338400000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:50.71 +54:41:18.2: 13.37 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:50.71 +54:41:18.2: 13.05 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 44 50.71 +54 41 18.2 11.7 U Cas 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 1994179536316071424,2461236.6591,11.72,0.05,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 1994179536316071424 20260715.1591 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 15.1591 2461236.6591 11.47 00:02:43.69 +50:56:32.7
115.14497 -11.19139 galactic Cas Second-epoch detections are separated by 3.6" and 9.2 pix
The object was found in VSX 2" Gaia DR3 394042878388217984
Type: ROT
# Max. Min./Amp. JD0 Period
13.220 G 13.270 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:43.69 +50:56:32.7: 13.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:43.69 +50:56:32.7: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 02 43.69 +50 56 32.7 11.5 U Cas 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 394042878388217984,2461236.6591,11.47,0.05,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 394042878388217984 20260715.1591 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.69 23:28:33.48 +53:36:16.9
110.71348 -7.28938 galactic Cas Second-epoch detections are separated by 0.8" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:33.48 +53:36:16.9 (user input) | T | P | (position from user input) J-Ks=0.863+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:33.48 +53:36:16.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:33.48 +53:36:16.9: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 28 33.48 +53 36 16.9 11.7 U Cas 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,2461236.6591,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.44 00:19:05.97 +56:05:25.5
118.40283 -6.49669 galactic Cas 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 | ATO J004.7658+56.1014 | 00:19:05.97 +56:05:25.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:05.97 +56:05:25.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:05.97 +56:05:25.5: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 19 05.97 +56 05 25.5 11.4 U Cas 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 J004.7658+56.1014,2461236.6591,11.44,0.05,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
ATO J004.7658+56.1014 20260715.1591 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 15.1591 2461236.6591 11.74 23:18:18.69 +56:19:02.6
110.23435 -4.24119 galactic Cas Second-epoch detections are separated by 1.3" 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 | ATO J349.5618+56.3050 | 23:18:18.91 +56:18:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:18.69 +56:19:02.6: 13.46 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:18.69 +56:19:02.6: 13.35 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 18 18.69 +56 19 02.6 11.7 U Cas 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 J349.5618+56.3050,2461236.6591,11.74,0.05,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
ATO J349.5618+56.3050 20260715.1591 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 15.1591 2461236.6591 11.32 00:01:46.28 +55:21:51.6
115.86206 -6.82418 galactic Cas Second-epoch detections are separated by 2.8" and 9.9 pix
The object was found in VSX16" Gaia DR3 420506645800207360
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.390 G 13.440 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:46.28 +55:21:51.6: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:46.28 +55:21:51.6: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 01 46.28 +55 21 51.6 11.3 U Cas 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 420506645800207360,2461236.6591,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420506645800207360 20260715.1591 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.63 23:30:17.89 +54:52:52.2
111.35996 -6.15721 galactic Cas Second-epoch detections are separated by 0.8" and 10.0 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 1997418766292819200 | 23:30:15.81 +54:52:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.362+/- (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:17.89 +54:52:52.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:17.89 +54:52:52.2: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 30 17.89 +54 52 52.2 11.6 U Cas 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 1997418766292819200,2461236.6591,11.63,0.05,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 1997418766292819200 20260715.1591 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.83 23:15:15.10 +52:14:45.7
108.34394 -7.88018 galactic And Second-epoch detections are separated by 2.8" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:15:15.10 +52:14:45.7 (user input) | T | P | (position from user input) J-Ks=0.540+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:15.10 +52:14:45.7: 13.55 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:15.10 +52:14:45.7: 13.09 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 15 15.10 +52 14 45.7 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461236.6591,11.83,0.05,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 20260715.1591 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 15.1591 2461236.6591 11.81 23:17:17.41 +55:07:46.7
109.67653 -5.30064 galactic Cas Second-epoch detections are separated by 2.0" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.3116+55.1290 | 23:17:17.41 +55:07:46.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.793+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:17.41 +55:07:46.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:17.41 +55:07:46.7: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 17 17.41 +55 07 46.7 11.8 U Cas 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 J349.3116+55.1290,2461236.6591,11.81,0.05,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
ATO J349.3116+55.1290 20260715.1591 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 15.1591 2461236.6591 11.71 23:12:47.14 +54:51:25.6
108.97259 -5.31858 galactic Cas Second-epoch detections are separated by 1.0" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.1994+54.8570 | 23:12:47.14 +54:51:25.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:47.14 +54:51:25.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:47.14 +54:51:25.6: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 12 47.14 +54 51 25.6 11.7 U Cas 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 J348.1994+54.8570,2461236.6591,11.71,0.05,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
ATO J348.1994+54.8570 20260715.1591 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 15.1591 2461236.6591 11.76 23:18:57.26 +55:20:51.0
109.97675 -5.18083 galactic Cas Second-epoch detections are separated by 1.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:57.26 +55:20:51.0 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.258+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:57.26 +55:20:51.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:57.26 +55:20:51.0: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 18 57.26 +55 20 51.0 11.8 U Cas 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,2461236.6591,11.76,0.05,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
target 20260715.1591 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 15.1591 2461236.6591 11.66 23:11:07.53 +55:23:54.3
108.95601 -4.72777 galactic Cas Second-epoch detections are separated by 3.0" and 10.7 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 J347.7659+55.4001 | 23:11:07.53 +55:23:54.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.513+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:07.53 +55:23:54.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:07.53 +55:23:54.3: 13.40 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 11 07.53 +55 23 54.3 11.7 U Cas 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 J347.7659+55.4001,2461236.6591,11.66,0.05,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
ATO J347.7659+55.4001 20260715.1591 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 15.1591 2461236.6591 11.51 23:35:27.44 +55:35:12.0
112.27846 -5.70559 galactic Cas Second-epoch detections are separated by 4.3" 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 1997479239433053696 | 23:35:24.49 +55:35:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:27.44 +55:35:12.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:27.44 +55:35:12.0: 13.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 35 27.44 +55 35 12.0 11.5 U Cas 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 1997479239433053696,2461236.6591,11.51,0.05,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 1997479239433053696 20260715.1591 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 15.1591 2461236.6591 11.46 23:36:53.20 +56:58:22.4
112.87023 -4.43536 galactic Cas Second-epoch detections are separated by 1.2" and 9.9 pix
The object was found in VSX 2" Gaia DR3 1998633211244654336
Type: ROT
# Max. Min./Amp. JD0 Period
13.210 G 13.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:53.20 +56:58:22.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:53.20 +56:58:22.4: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 36 53.20 +56 58 22.4 11.5 U Cas 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 1998633211244654336,2461236.6591,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998633211244654336 20260715.1591 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.57 23:15:56.70 +52:27:18.5
108.52043 -7.72411 galactic And Second-epoch detections are separated by 0.9" and 10.5 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 J348.9641+52.4446 | 23:15:51.81 +52:27:08.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.849+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:56.70 +52:27:18.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:56.70 +52:27:18.5: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 15 56.70 +52 27 18.5 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.9641+52.4446,2461236.6591,11.57,0.05,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 J348.9641+52.4446 20260715.1591 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 15.1591 2461236.6591 11.17 00:14:57.02 +55:03:50.7
117.67875 -7.43507 galactic Cas 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 | Large-amplitude variable Gaia DR2 420570108229652736 | 00:14:57.02 +55:03:50.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G5 (LAMOST DR5) J-Ks=0.770+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:57.02 +55:03:50.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:57.02 +55:03:50.7: 13.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 14 57.02 +55 03 50.7 11.2 U Cas 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 420570108229652736,2461236.6591,11.17,0.05,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 420570108229652736 20260715.1591 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.29 23:18:41.19 +54:16:18.5
109.56027 -6.17424 galactic Cas Second-epoch detections are separated by 1.9" and 10.4 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 1995973075999277440 | 23:18:38.04 +54:16:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.721+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:41.19 +54:16:18.5: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:41.19 +54:16:18.5: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 18 41.19 +54 16 18.5 11.3 U Cas 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 1995973075999277440,2461236.6591,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995973075999277440 20260715.1591 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 15.1591 2461236.6591 11.32 23:22:17.57 +56:46:56.9
110.91164 -3.99435 galactic Cas Second-epoch detections are separated by 1.0" and 10.1 pix
The object was found in VSX 1" Gaia DR3 1997307028422503296
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.900 G 12.980 G 0.142002300000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:17.57 +56:46:56.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:17.57 +56:46:56.9: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 22 17.57 +56 46 56.9 11.3 U Cas 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 1997307028422503296,2461236.6591,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997307028422503296 20260715.1591 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.01 23:58:40.05 +53:54:14.7
115.12510 -8.16586 galactic Cas Second-epoch detections are separated by 1.5" 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 J359.6649+53.9052 | 23:58:40.05 +53:54:14.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:40.05 +53:54:14.7: 13.24 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:40.05 +53:54:14.7: 13.16 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 58 40.05 +53 54 14.7 11.0 U Cas 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 J359.6649+53.9052,2461236.6591,11.01,0.05,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 J359.6649+53.9052 20260715.1591 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.24 23:28:23.21 +57:13:12.9
111.84111 -3.85228 galactic Cas Second-epoch detections are separated by 0.6" and 10.0 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 1998829370990757376 | 23:28:25.30 +57:13:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:23.21 +57:13:12.9: 13.62 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:23.21 +57:13:12.9: 13.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.62 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 28 23.21 +57 13 12.9 11.2 U Cas 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 1998829370990757376,2461236.6591,11.24,0.05,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 1998829370990757376 20260715.1591 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.07 23:39:41.88 +57:16:03.1
113.32032 -4.25937 galactic Cas Second-epoch detections are separated by 0.8" and 9.8 pix
The object was found in VSX21" Gaia DR3 1998666952508357760
Type: ROT
# Max. Min./Amp. JD0 Period
14.090 G 14.120 G K
ATTENTION: measured mag 11.07 is 3.0 mag brighter than the VSX record maximum brightness 14.09 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:41.88 +57:16:03.1: 13.56 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:41.88 +57:16:03.1: 13.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.56 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 39 41.88 +57 16 03.1 11.1 U Cas 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 1998666952508357760,2461236.6591,11.07,0.05,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 1998666952508357760 20260715.1591 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 15.1591 2461236.6591 11.01 23:25:58.47 +50:16:18.4
109.24125 -10.31435 galactic And Second-epoch detections are separated by 2.3" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:58.47 +50:16:18.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:58.47 +50:16:18.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:58.47 +50:16:18.4: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 25 58.47 +50 16 18.4 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461236.6591,11.01,0.05,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 20260715.1591 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.24 23:12:41.21 +54:49:12.9
108.94552 -5.34746 galactic Cas Second-epoch detections are separated by 0.7" and 10.4 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 1996494626770732160 | 23:12:37.83 +54:49:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.21 +54:49:12.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:41.21 +54:49:12.9: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 12 41.21 +54 49 12.9 11.2 U Cas 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 1996494626770732160,2461236.6591,11.24,0.05,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 1996494626770732160 20260715.1591 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.15 23:13:08.84 +53:45:18.4
108.60896 -6.36085 galactic Cas Second-epoch detections are separated by 1.3" and 10.1 pix
The object was found in VSX 3" ZTF J231308.58+534520.0
Type: M
# Max. Min./Amp. JD0 Period
19.454 g Y 4.908 g 2458360.34240 358.008827700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:08.84 +53:45:18.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:08.84 +53:45:18.4: 13.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 13 08.84 +53 45 18.4 11.2 U Cas 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
ZTF J231308.58+534520.0,2461236.6591,11.15,0.05,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
ZTF J231308.58+534520.0 20260715.1591 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 15.1591 2461236.6591 11.05 23:10:02.51 +56:51:40.2
109.37335 -3.31741 galactic Cas Second-epoch detections are separated by 0.4" and 10.4 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 J347.5055+56.8648 | 23:10:04.48 +56:52:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.271+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:02.51 +56:51:40.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:02.51 +56:51:40.2: 13.36 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 10 02.51 +56 51 40.2 11.1 U Cas 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 J347.5055+56.8648,2461236.6591,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5055+56.8648 20260715.1591 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 10.13 23:50:25.84 +49:51:13.2
112.95281 -11.83233 galactic Cas Second-epoch detections are separated by 1.5" 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 1940880469640450304 | 23:50:26.96 +49:51:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.045+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:25.84 +49:51:13.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:25.84 +49:51:13.2: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 50 25.84 +49 51 13.2 10.1 U Cas 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 1940880469640450304,2461236.6591,10.13,0.05,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 1940880469640450304 20260715.1591 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 9.91 23:27:26.44 +49:36:03.3
109.24471 -11.02547 galactic And Second-epoch detections are separated by 1.3" and 10.4 pix
The object was not found in VSX
The object was found in ASASSN-V 3" ASASSN-V J232726.19+493602.3
Type: L
MeanMag 11.8 m Amp. 0.09 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:26.44 +49:36:03.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:26.44 +49:36:03.3: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 27 26.44 +49 36 03.3 9.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461236.6591,9.91,0.05,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
VARIABLE_NAME 20260715.1591 9.91CV 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 15.1591 2461236.6591 9.89 23:36:32.65 +50:40:32.9
110.99395 -10.45182 galactic And Second-epoch detections are separated by 1.7" and 10.2 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 1944540365891633792 | 23:36:31.17 +50:40:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:32.65 +50:40:32.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:32.65 +50:40:32.9: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 36 32.65 +50 40 32.9 9.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944540365891633792,2461236.6591,9.89,0.05,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
Gaia DR3 1944540365891633792 20260715.1591 9.89CV 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 15.1591 2461236.6591 9.57 23:22:01.62 +54:00:51.3
109.93217 -6.58538 galactic Cas Second-epoch detections are separated by 0.5" and 10.2 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 1995778913417432832 | 23:22:03.08 +54:01:06.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.059+/-0.035 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:01.62 +54:00:51.3: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:01.62 +54:00:51.3: 13.34 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 22 01.62 +54 00 51.3 9.6 U Cas 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 1995778913417432832,2461236.6591,9.57,0.05,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 1995778913417432832 20260715.1591 9.57CV 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 15.1591 2461236.6591 10.08 23:20:57.79 +55:40:10.6
110.35679 -4.97752 galactic Cas Second-epoch detections are separated by 0.3" and 10.1 pix
The object was found in VSX16" Gaia DR3 1996906600032621824
Type: ROT
# Max. Min./Amp. JD0 Period
14.660 G 14.690 G F
ATTENTION: measured mag 10.08 is 4.6 mag brighter than the VSX record maximum brightness 14.66 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:57.79 +55:40:10.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:57.79 +55:40:10.6: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 20 57.79 +55 40 10.6 10.1 U Cas 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 1996906600032621824,2461236.6591,10.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996906600032621824 20260715.1591 10.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.05 23:23:03.73 +55:52:05.7
110.70319 -4.89100 galactic Cas Second-epoch detections are separated by 0.9" and 10.2 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 J350.7593+55.8722 | 23:23:05.90 +55:52:41.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1928AnHar.100...49C HD 240277 J-Ks=0.843+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:03.73 +55:52:05.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:03.73 +55:52:05.7: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 23 03.73 +55 52 05.7 11.1 U Cas 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 J350.7593+55.8722,2461236.6591,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.7593+55.8722 20260715.1591 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.01 23:22:36.60 +57:23:00.6
111.15566 -3.44317 galactic Cas Second-epoch detections are separated by 0.3" and 10.2 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 2009390970447326080 | 23:22:32.69 +57:22:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.745+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:36.60 +57:23:00.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:36.60 +57:23:00.6: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 22 36.60 +57 23 00.6 11.0 U Cas 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 2009390970447326080,2461236.6591,11.01,0.05,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 2009390970447326080 20260715.1591 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.06 23:18:56.62 +53:20:37.2
109.26684 -7.05624 galactic Cas Second-epoch detections are separated by 0.9" and 10.1 pix
The object was found in VSX 2" Gaia DR3 1995687275993223168
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.62 +53:20:37.2: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:56.62 +53:20:37.2: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 18 56.62 +53 20 37.2 11.1 U Cas 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 1995687275993223168,2461236.6591,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995687275993223168 20260715.1591 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.15 23:13:38.90 +53:34:20.0
108.60991 -6.55822 galactic Cas Second-epoch detections are separated by 0.3" and 10.3 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 1995573094286898944 | 23:13:35.10 +53:34:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.475+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:38.90 +53:34:20.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:38.90 +53:34:20.0: 13.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 13 38.90 +53 34 20.0 11.2 U Cas 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 1995573094286898944,2461236.6591,11.15,0.05,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
Gaia DR3 1995573094286898944 20260715.1591 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 15.1591 2461236.6591 11.12 23:28:46.75 +52:18:45.2
110.33116 -8.52523 galactic Cas Second-epoch detections are separated by 0.1" and 10.2 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 1991700068875645312 | 23:28:50.45 +52:18:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:46.75 +52:18:45.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:46.75 +52:18:45.2: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 28 46.75 +52 18 45.2 11.1 U Cas 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 1991700068875645312,2461236.6591,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991700068875645312 20260715.1591 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.18 23:29:36.54 +50:10:57.3
109.77136 -10.58653 galactic And Second-epoch detections are separated by 0.7" and 10.4 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 1943178620739712384 | 23:29:33.48 +50:10:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.471+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:36.54 +50:10:57.3: 13.33 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:36.54 +50:10:57.3: 13.04 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 29 36.54 +50 10 57.3 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943178620739712384,2461236.6591,11.18,0.05,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 1943178620739712384 20260715.1591 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.54 23:12:17.73 +57:05:10.2
109.74326 -3.22506 galactic Cas Second-epoch detections are separated by 2.4" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.0943+57.0885 | 23:12:17.73 +57:05:10.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.73 +57:05:10.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.73 +57:05:10.2: 13.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 12 17.73 +57 05 10.2 11.5 U Cas 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 J348.0943+57.0885,2461236.6591,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.0943+57.0885 20260715.1591 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.51 23:23:47.54 +54:34:20.7
110.36563 -6.14684 galactic Cas Second-epoch detections are separated by 0.6" and 10.1 pix
The object was found in VSX 1" ZTF J232347.55+543421.8
Type: SR
# Max. Min./Amp. JD0 Period
12.954 r Y 0.042 r 2458657.89370 34.975481300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:47.54 +54:34:20.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:47.54 +54:34:20.7: 13.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 23 47.54 +54 34 20.7 11.5 U Cas 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
ZTF J232347.55+543421.8,2461236.6591,11.51,0.05,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
ZTF J232347.55+543421.8 20260715.1591 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 15.1591 2461236.6591 11.59 23:19:32.25 +55:36:22.9
110.14536 -4.96723 galactic Cas Second-epoch detections are separated by 3.8" and 10.8 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 1996916972372159360 | 23:19:35.92 +55:36:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:32.25 +55:36:22.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:32.25 +55:36:22.9: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 19 32.25 +55 36 22.9 11.6 U Cas 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 1996916972372159360,2461236.6591,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996916972372159360 20260715.1591 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.48 23:19:47.78 +49:05:02.6
107.87265 -11.08954 galactic And Second-epoch detections are separated by 0.9" and 10.5 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 J349.9432+49.0855 | 23:19:50.31 +49:05:32.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.379+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:47.78 +49:05:02.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:47.78 +49:05:02.6: 13.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 19 47.78 +49 05 02.6 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.9432+49.0855,2461236.6591,11.48,0.05,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
ATO J349.9432+49.0855 20260715.1591 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 15.1591 2461236.6591 11.78 23:11:51.71 +55:18:27.8
109.01894 -4.85125 galactic Cas Second-epoch detections are separated by 3.5" and 10.0 pix
The object was found in VSX 4" Gaia DR3 1996757100812082688
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.560 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.71 +55:18:27.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.71 +55:18:27.8: 13.51 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 11 51.71 +55 18 27.8 11.8 U Cas 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 1996757100812082688,2461236.6591,11.78,0.05,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 1996757100812082688 20260715.1591 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 15.1591 2461236.6591 11.62 23:23:13.30 +52:06:49.9
109.45216 -8.43395 galactic And Second-epoch detections are separated by 2.4" and 10.0 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 1992342699061284736 | 23:23:09.69 +52:06:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:13.30 +52:06:49.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:13.30 +52:06:49.9: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 23 13.30 +52 06 49.9 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992342699061284736,2461236.6591,11.62,0.05,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 1992342699061284736 20260715.1591 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 15.1591 2461236.6591 11.75 23:25:28.04 +49:20:10.3
108.84749 -11.17012 galactic And Second-epoch detections are separated by 1.5" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:28.04 +49:20:10.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.04 +49:20:10.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:28.04 +49:20:10.3: 13.42 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 15.1591* 23 25 28.04 +49 20 10.3 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461236.6591,11.75,0.05,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 20260715.1591 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.50 00:03:27.64 +55:39:37.5
116.15496 -6.57877 galactic Cas Second-epoch detections are separated by 2.5" 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 | 00:03:27.64 +55:39:37.5 (user input) | T | P | (position from user input) J-Ks=13.273+/- (unrealisitic color!)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:27.64 +55:39:37.5: 13.35 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:27.64 +55:39:37.5: 12.70 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 03 27.64 +55 39 37.5 11.5 U Cas 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,2461236.6591,11.50,0.05,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 20260715.1591 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.93 23:13:21.35 +55:04:15.2
109.12871 -5.15057 galactic Cas Second-epoch detections are separated by 0.9" and 10.3 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 1996689412126188928 | 23:13:23.53 +55:04:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:21.35 +55:04:15.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:21.35 +55:04:15.2: 13.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 13 21.35 +55 04 15.2 11.9 U Cas 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 1996689412126188928,2461236.6591,11.93,0.05,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 1996689412126188928 20260715.1591 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 15.1591 2461236.6591 11.85 23:17:28.98 +54:27:12.1
109.46017 -5.94232 galactic Cas Second-epoch detections are separated by 2.1" and 10.5 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 J349.3716+54.4392 | 23:17:30.61 +54:26:43.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:28.98 +54:27:12.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:28.98 +54:27:12.1: 13.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 17 28.98 +54 27 12.1 11.8 U Cas 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 J349.3716+54.4392,2461236.6591,11.85,0.05,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
ATO J349.3716+54.4392 20260715.1591 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 15.1591 2461236.6591 11.90 23:21:16.93 +54:35:02.7
110.02543 -6.01273 galactic Cas Second-epoch detections are separated by 2.0" and 10.2 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 1996006855921682048 | 23:21:15.41 +54:34:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:16.93 +54:35:02.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:16.93 +54:35:02.7: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 21 16.93 +54 35 02.7 11.9 U Cas 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 1996006855921682048,2461236.6591,11.90,0.05,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
Gaia DR3 1996006855921682048 20260715.1591 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 15.1591 2461236.6591 11.67 23:42:14.37 +51:45:06.4
112.16909 -9.66806 galactic Cas 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 | 23:42:14.37 +51:45:06.4 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:14.37 +51:45:06.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:14.37 +51:45:06.4: 13.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 42 14.37 +51 45 06.4 11.7 U Cas 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,2461236.6591,11.67,0.05,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
target 20260715.1591 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 15.1591 2461236.6591 11.73 23:29:24.02 +51:39:58.4
110.21579 -9.16858 galactic Cas Second-epoch detections are separated by 2.2" and 10.3 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 | Large-amplitude variable Gaia DR2 1991424538127002368 | 23:29:24.02 +51:39:58.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.02 +51:39:58.4: 13.23 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:24.02 +51:39:58.4: 13.05 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 29 24.02 +51 39 58.4 11.7 U Cas 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 1991424538127002368,2461236.6591,11.73,0.05,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
Large-amplitude variable Gaia DR2 1991424538127002368 20260715.1591 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 15.1591 2461236.6591 11.82 23:34:08.18 +54:02:57.8
111.64069 -7.11902 galactic Cas Second-epoch detections are separated by 0.7" and 9.9 pix
The object was found in VSX 1" Gaia DR3 1994286807419596416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.630 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.18 +54:02:57.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.18 +54:02:57.8: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 34 08.18 +54 02 57.8 11.8 U Cas 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 1994286807419596416,2461236.6591,11.82,0.05,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 1994286807419596416 20260715.1591 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 15.1591 2461236.6591 11.64 00:11:12.94 +57:36:26.1
117.54543 -4.84323 galactic Cas Second-epoch detections are separated by 1.9" 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 | ATO J002.8033+57.5971 | 00:11:12.94 +57:36:26.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:12.94 +57:36:26.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:12.94 +57:36:26.1: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 11 12.94 +57 36 26.1 11.6 U Cas 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 J002.8033+57.5971,2461236.6591,11.64,0.05,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
ATO J002.8033+57.5971 20260715.1591 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 15.1591 2461236.6591 11.90 23:24:53.15 +54:29:06.4
110.48698 -6.28187 galactic Cas Second-epoch detections are separated by 1.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:53.15 +54:29:06.4 (user input) | T | P | (position from user input) J-Ks=0.790+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:53.15 +54:29:06.4: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:53.15 +54:29:06.4: 13.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 24 53.15 +54 29 06.4 11.9 U Cas 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,2461236.6591,11.90,0.05,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 20260715.1591 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 15.1591 2461236.6591 11.67 23:41:49.97 +54:40:27.0
112.90193 -6.83642 galactic Cas Second-epoch detections are separated by 1.1" 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 | ATO J355.4769+54.6722 | 23:41:49.97 +54:40:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.736+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:49.97 +54:40:27.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:49.97 +54:40:27.0: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 41 49.97 +54 40 27.0 11.7 U Cas 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 J355.4769+54.6722,2461236.6591,11.67,0.05,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
ATO J355.4769+54.6722 20260715.1591 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 15.1591 2461236.6591 11.68 23:30:32.31 +49:52:17.5
109.81588 -10.92876 galactic And Second-epoch detections are separated by 1.7" and 10.4 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 J352.6481+49.8736 | 23:30:33.67 +49:52:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:32.31 +49:52:17.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:32.31 +49:52:17.5: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 30 32.31 +49 52 17.5 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.6481+49.8736,2461236.6591,11.68,0.05,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
ATO J352.6481+49.8736 20260715.1591 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 15.1591 2461236.6591 12.09 23:22:37.39 +57:23:26.7
111.15978 -3.43694 galactic Cas Second-epoch detections are separated by 4.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:22:37.39 +57:23:26.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:37.39 +57:23:26.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:37.39 +57:23:26.7: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 22 37.39 +57 23 26.7 12.1 U Cas 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,2461236.6591,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260715.1591 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 12.06 23:14:32.72 +54:34:06.2
109.10247 -5.68083 galactic Cas Second-epoch detections are separated by 2.1" 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 | ATO J348.6167+54.5671 | 23:14:32.72 +54:34:06.2 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:32.72 +54:34:06.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:32.72 +54:34:06.2: 13.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 14 32.72 +54 34 06.2 12.1 U Cas 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 J348.6167+54.5671,2461236.6591,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.6167+54.5671 20260715.1591 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 15.1591 2461236.6591 11.91 23:56:18.84 +57:40:50.0
115.59325 -4.40363 galactic Cas Second-epoch detections are separated by 3.3" 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 | 23:56:18.84 +57:40:50.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:18.84 +57:40:50.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:18.84 +57:40:50.0: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 56 18.84 +57 40 50.0 11.9 U Cas 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,2461236.6591,11.91,0.05,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 20260715.1591 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 15.1591 2461236.6591 11.87 23:25:37.60 +52:09:11.4
109.81719 -8.51997 galactic And Second-epoch detections are separated by 0.5" and 10.2 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 1992422894689901952 | 23:25:33.01 +52:08:58.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:37.60 +52:09:11.4: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:37.60 +52:09:11.4: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 25 37.60 +52 09 11.4 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992422894689901952,2461236.6591,11.87,0.05,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 1992422894689901952 20260715.1591 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 15.1591 2461236.6591 11.92 23:32:21.34 +53:10:39.4
111.12253 -7.87122 galactic Cas Second-epoch detections are separated by 0.4" and 10.2 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 J353.0827+53.1779 | 23:32:21.34 +53:10:39.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.855+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:21.34 +53:10:39.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:21.34 +53:10:39.4: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 32 21.34 +53 10 39.4 11.9 U Cas 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 J353.0827+53.1779,2461236.6591,11.92,0.05,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
ATO J353.0827+53.1779 20260715.1591 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 15.1591 2461236.6591 11.99 23:24:34.88 +53:01:03.4
109.95456 -7.65165 galactic And Second-epoch detections are separated by 2.0" and 10.0 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 1992707565122670464 | 23:24:38.53 +53:01:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.750+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:34.88 +53:01:03.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:34.88 +53:01:03.4: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 24 34.88 +53 01 03.4 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992707565122670464,2461236.6591,11.99,0.05,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 1992707565122670464 20260715.1591 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.95 23:28:53.99 +52:19:34.6
110.35325 -8.51807 galactic Cas Second-epoch detections are separated by 2.8" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.2084+52.3397 | 23:28:50.12 +52:19:40.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:53.99 +52:19:34.6: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:53.99 +52:19:34.6: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 28 53.99 +52 19 34.6 11.9 U Cas 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 J352.2084+52.3397,2461236.6591,11.95,0.05,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
ATO J352.2084+52.3397 20260715.1591 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 15.1591 2461236.6591 11.90 23:44:00.32 +53:01:54.5
112.77533 -8.50502 galactic Cas Second-epoch detections are separated by 0.4" 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 | ATO J355.9935+53.0252 | 23:44:00.32 +53:01:54.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.266+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:00.32 +53:01:54.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:00.32 +53:01:54.5: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 44 00.32 +53 01 54.5 11.9 U Cas 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 J355.9935+53.0252,2461236.6591,11.90,0.05,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
ATO J355.9935+53.0252 20260715.1591 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 15.1591 2461236.6591 12.01 23:17:29.49 +52:31:58.0
108.77026 -7.73661 galactic And Second-epoch detections are separated by 2.4" and 10.6 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 1992633451161006720 | 23:17:33.26 +52:31:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.271+/-0.044 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:29.49 +52:31:58.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:29.49 +52:31:58.0: 13.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 17 29.49 +52 31 58.0 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992633451161006720,2461236.6591,12.01,0.05,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 1992633451161006720 20260715.1591 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.71 00:04:53.84 +51:59:43.8
115.68299 -10.21999 galactic Cas Second-epoch detections are separated by 4.1" 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 | ATO J001.2174+52.0011 | 00:04:53.84 +51:59:43.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.84 +51:59:43.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:53.84 +51:59:43.8: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 00 04 53.84 +51 59 43.8 11.7 U Cas 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 J001.2174+52.0011,2461236.6591,11.71,0.05,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
ATO J001.2174+52.0011 20260715.1591 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 15.1591 2461236.6591 12.06 23:22:00.12 +53:55:31.1
109.89817 -6.66774 galactic Cas Second-epoch detections are separated by 2.1" and 10.2 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 J350.4863+53.9214 | 23:21:56.73 +53:55:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:00.12 +53:55:31.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:00.12 +53:55:31.1: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 22 00.12 +53 55 31.1 12.1 U Cas 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 J350.4863+53.9214,2461236.6591,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.4863+53.9214 20260715.1591 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 15.1591 2461236.6591 12.40 23:31:12.15 +56:29:06.0
111.97843 -4.67079 galactic Cas Second-epoch detections are separated by 1.4" and 10.2 pix
The object was found in VSX 3" WISE J233112.3+562908
Type: EW
# Max. Min./Amp. JD0 Period
14.288 r Y 0.237 r 2458362.84430 0.315021200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:12.15 +56:29:06.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:12.15 +56:29:06.0: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 31 12.15 +56 29 06.0 12.4 U Cas 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
WISE J233112.3+562908,2461236.6591,12.40,0.05,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
WISE J233112.3+562908 20260715.1591 12.40CV 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 15.1591 2461236.6591 12.50 23:14:46.47 +54:27:10.7
109.09105 -5.80040 galactic Cas Second-epoch detections are separated by 0.8" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:14:46.47 +54:27:10.7 (user input) | T | P | (position from user input) J-Ks=0.766+/-0.037 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.47 +54:27:10.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:46.47 +54:27:10.7: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 14 46.47 +54 27 10.7 12.5 U Cas 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,2461236.6591,12.50,0.05,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 20260715.1591 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 15.1591 2461236.6591 11.45 23:26:01.31 +49:55:45.8
109.13376 -10.64010 galactic And Second-epoch detections are separated by 0.8" and 10.3 pix
The object was found in VSX 3" Gaia DR3 1943087155117309568
Type:
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:01.31 +49:55:45.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:01.31 +49:55:45.8: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 26 01.31 +49 55 45.8 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943087155117309568,2461236.6591,11.45,0.05,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 1943087155117309568 20260715.1591 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 15.1591 2461236.6591 10.97 23:21:12.03 +50:00:11.7
108.41725 -10.30823 galactic And Second-epoch detections are separated by 1.8" and 10.6 pix
The object was found in VSX 4" AK And
Type: M
# Max. Min./Amp. JD0 Period
10.000 V < 15.000 V 2452930.00000 317.000000000000 S:
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:12.03 +50:00:11.7: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:12.03 +50:00:11.7: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 15.1591* 23 21 12.03 +50 00 11.7 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AK And,2461236.6591,10.97,0.05,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
AK And 20260715.1591 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461236.65955975 15.07.2026 03:49:35.962 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 28 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): 21618
Objects passed selection criteria: 21577
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 18337
Average stars matched: 17382 (94.792 %)
Memory usage VmPeak: 131328 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jul 13 18:59:08 CDT 2026
VaST build number 1.0rc89-151-g9f3411f7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 15 00:17:36 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461236.65955975 15.07.2026 03:49:35.962 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 294
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 738 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): 162974
Objects passed selection criteria: 162595
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 143753
Average stars matched: 136854 (95.2003 %)
Memory usage VmPeak: 1998076 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jul 13 18:59:08 CDT 2026
VaST build number 1.0rc89-151-g9f3411f7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 15 00:34:25 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 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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: 2461236.65868008
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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Image size: 940.2'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.051 +53:59:54.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.051 +53:59:54.12
Angular distance between the image centers 0.0232 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Image size: 940.1'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:06.370 +53:59:10.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:06.370 +53:59:10.20
Angular distance between the image centers 0.0391 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:02.051 +53:59:54.12
Second-epoch second image center 00:00:06.370 +53:59:10.20
Angular distance between the image centers 0.01615 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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.LP8d49bmpO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.u4l0YmVbRw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits &> /tmp/tmp.rkhP72aRrP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits &> /tmp/tmp.45qpkYwc2K
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
ERROR: only 52 of 28951 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.18%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.575300
a=0.000000 b=1.000000 c=22.575300
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
Read 32399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0011 to 359.9996 deg, Dec +48.2682 to +59.2618 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0011 to 359.9996 deg, Dec 48.2682 to 59.2618 deg
Loaded 153285 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): 56 out of 62 total matches.
Matched with Tycho-2 62 out of 32399 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.0 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (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.LP8d49bmpO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0821 through 0 to 14.9840, gap 14.9840 to 345.0821
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 235 matched stars entering correct_measured_positions(), 5819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.02"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0724 through 0 to 15.0101, gap 15.0101 to 345.0724
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 401 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 345 matched stars entering correct_measured_positions(), 5883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.97"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.85"
Excluding outliers - 341 stars left (next iteration limit 258)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.000 sigma_q1_arcsec=26.458 sigma_q2_arcsec=26.280 sigma_q3_arcsec=7.321 sigma_q4_arcsec=8.000 n_q1=41 n_q2=24 n_q3=122 n_q4=154 worst_quadrant_to_overall_ratio=2.646
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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.u4l0YmVbRw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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=3204, bad_region=7312, passed=32399
Got 32399 stars (including 22421 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 32399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0823 through 0 to 14.9840, gap 14.9840 to 345.0823
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 320 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 234 matched stars entering correct_measured_positions(), 171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 6406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0732 through 0 to 15.0096, gap 15.0096 to 345.0732
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 399 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 343 matched stars entering correct_measured_positions(), 6467 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.48"
Accuracy estimation diagnostic: 340 matched stars entering correct_measured_positions(), 9572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.44"
Excluding outliers - 340 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=340 sigma_overall_arcsec=11.206 sigma_q1_arcsec=29.679 sigma_q2_arcsec=28.591 sigma_q3_arcsec=8.393 sigma_q4_arcsec=9.911 n_q1=41 n_q2=25 n_q3=115 n_q4=159 worst_quadrant_to_overall_ratio=2.649
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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.rkhP72aRrP (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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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=1114, bad_region=2686, passed=16002
Got 16002 stars (including 12339 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 16002 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.2'
Seting catalog search parameters based on the expected field of view 940.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013058 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010447 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8481 through 0 to 14.6565, gap 14.6565 to 344.8481
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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: 972 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 13551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8494 through 0 to 14.6572, gap 14.6572 to 344.8494
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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: 972 matched stars entering correct_measured_positions(), 13551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 13551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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=fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits N_match=972 sigma_overall_arcsec=0.683 sigma_q1_arcsec=0.745 sigma_q2_arcsec=0.878 sigma_q3_arcsec=0.660 sigma_q4_arcsec=0.692 n_q1=319 n_q2=163 n_q3=301 n_q4=189 worst_quadrant_to_overall_ratio=1.284
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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.45qpkYwc2K (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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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=1144, bad_region=2757, passed=16051
Got 16051 stars (including 12283 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 16051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.1'
Seting catalog search parameters based on the expected field of view 940.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013057 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010446 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8680 through 0 to 14.6558, gap 14.6558 to 344.8680
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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: 972 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 13523 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8692 through 0 to 14.6565, gap 14.6565 to 344.8692
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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: 972 matched stars entering correct_measured_positions(), 13522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 13522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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=fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits N_match=972 sigma_overall_arcsec=0.749 sigma_q1_arcsec=0.769 sigma_q2_arcsec=0.889 sigma_q3_arcsec=0.693 sigma_q4_arcsec=0.711 n_q1=324 n_q2=165 n_q3=293 n_q4=190 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits sigma_overall=10.000 worst_q_ratio=2.646
ref2=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits sigma_overall=11.206 worst_q_ratio=2.649
new1=fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits sigma_overall=0.683 worst_q_ratio=1.284
new2=fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits sigma_overall=0.749 worst_q_ratio=1.186
reference average sigma_overall=10.603 worst_q_ratio=2.6475
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (341 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.98 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450_astrometric_residuals.png (340 matched stars from wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.94 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.68 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:43.52 +56:37:02.6: 14.90 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:30.26 +53:14:07.2: 13.51 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:30.26 +53:14:07.2: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter KEPT candidate at 23:19:30.26 +53:14:07.2: ref_mag=13.53 +/- 0.04 new_mean_mag=11.8739 delta=1.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:43.52 +56:37:02.6: 15.14 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.17
Forced photometry filter KEPT candidate at 23:38:43.52 +56:37:02.6: ref_mag=15.01 +/- 0.17 new_mean_mag=11.0746 delta=3.93 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out33558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33560.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 33558_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 33558_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:19:30.26 +53:14:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.405 1995670577160414720 349.87551833397 +53.23552829053 11.5770 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 33560_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 33560_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:38:43.52 +56:37:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 0.717 1997852794203517824 354.68124988326 +56.61758278250 10.9060 10.3872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 21482_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:31.89 +56:34:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 06239_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:58:25.14 +51:23:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 07077_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:09:36.49 +51:34:01.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Cas-04-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 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Image size: 940.2'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.051 +53:59:54.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.051 +53:59:54.12
Angular distance between the image centers 0.0232 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Image size: 940.1'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:06.370 +53:59:10.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:06.370 +53:59:10.20
Angular distance between the image centers 0.0391 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:02.051 +53:59:54.12
Second-epoch second image center 00:00:06.370 +53:59:10.20
Angular distance between the image centers 0.01615 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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.Kp18kn6Zbj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.NZCAiXfoYi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits &> /tmp/tmp.Ze0nE5y6dv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits &> /tmp/tmp.rQsadZhR3H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
ERROR: only 104 of 200953 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.05%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.521000
a=0.000000 b=1.000000 c=20.521000
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.21
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=4.7)
Read 213202 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9999 deg, Dec +48.2308 to +59.2649 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0002 to 359.9999 deg, Dec 48.2308 to 59.2649 deg
Loaded 153847 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): 122 out of 166 total matches.
Matched with Tycho-2 166 out of 213202 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 223 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
13.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
13.3 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
12.6 mag. fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
12.6 mag. fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.0 (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.Kp18kn6Zbj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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=60, blended=29230, bad_region=30798, passed=200893
Got 200893 stars (including 144443 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 200893 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0121 through 0 to 15.0290, gap 15.0290 to 345.0121
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 42039 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0161 through 0 to 15.0639, gap 15.0639 to 345.0161
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 402 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 42110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.32"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 65834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.71"
Excluding outliers - 341 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.173 sigma_q1_arcsec=28.653 sigma_q2_arcsec=29.926 sigma_q3_arcsec=7.272 sigma_q4_arcsec=10.943 n_q1=31 n_q2=26 n_q3=117 n_q4=167 worst_quadrant_to_overall_ratio=2.942
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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.NZCAiXfoYi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=33709, bad_region=29431, passed=213150
Got 213150 stars (including 154424 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 213150 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0123 through 0 to 15.0317, gap 15.0317 to 345.0123
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 319 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 46390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0158 through 0 to 15.0663, gap 15.0663 to 345.0158
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 46448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.44"
Accuracy estimation diagnostic: 332 matched stars entering correct_measured_positions(), 66751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.69"
Excluding outliers - 332 stars left (next iteration limit 249)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=332 sigma_overall_arcsec=11.113 sigma_q1_arcsec=28.693 sigma_q2_arcsec=26.729 sigma_q3_arcsec=8.129 sigma_q4_arcsec=9.837 n_q1=36 n_q2=26 n_q3=118 n_q4=152 worst_quadrant_to_overall_ratio=2.582
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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.Ze0nE5y6dv (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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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=21, blended=12300, bad_region=14773, passed=126140
Got 126140 stars (including 99999 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 126140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.2'
Seting catalog search parameters based on the expected field of view 940.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013058 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010447 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.7708 through 0 to 14.7935, gap 14.7935 to 344.7708
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 112938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.7704 through 0 to 14.7942, gap 14.7942 to 344.7704
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 112938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 112939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits N_match=975 sigma_overall_arcsec=0.692 sigma_q1_arcsec=0.717 sigma_q2_arcsec=0.808 sigma_q3_arcsec=0.692 sigma_q4_arcsec=0.719 n_q1=334 n_q2=159 n_q3=286 n_q4=196 worst_quadrant_to_overall_ratio=1.168
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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.rQsadZhR3H (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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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=29, blended=12116, bad_region=15023, passed=127878
Got 127878 stars (including 101752 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 127878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.1'
Seting catalog search parameters based on the expected field of view 940.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013057 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010446 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8681 through 0 to 14.7916, gap 14.7916 to 344.8681
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 114567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8692 through 0 to 14.7922, gap 14.7922 to 344.8692
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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(), 114568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 114569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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=fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits N_match=972 sigma_overall_arcsec=0.727 sigma_q1_arcsec=0.719 sigma_q2_arcsec=0.845 sigma_q3_arcsec=0.693 sigma_q4_arcsec=0.738 n_q1=330 n_q2=168 n_q3=284 n_q4=190 worst_quadrant_to_overall_ratio=1.163
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-48-19_20.00sec_5.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.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_2026-07-14_CI_Cas-04-Q2b1x1_225157_TTUQ2b1x1_1569890_8U9O2vA7/wcs_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:35.78 +56:31:47.5: 12.13 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:25.08 +51:16:42.3: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:33.09 +53:02:41.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:49.01 +51:38:40.2: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:13.25 +57:06:48.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:44.91 +53:08:11.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:30.37 +54:23:52.2: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:09.41 +56:23:37.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:07.64 +54:31:56.6: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:22.11 +53:12:39.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:25.08 +51:16:42.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:13.25 +57:06:48.2: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:33.09 +53:02:41.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:44.91 +53:08:11.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:30.37 +54:23:52.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:09.41 +56:23:37.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:49.01 +51:38:40.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:07.64 +54:31:56.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:35.78 +56:31:47.5: 12.12 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:22.11 +53:12:39.3: 13.57 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.13 +/- 0.06
Forced photometry filter REJECTED candidate at 23:56:35.78 +56:31:47.5: ref_mag=12.13 +/- 0.06 new_mean_mag=12.2688 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:29.16 +54:40:20.3: 13.45 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:29.16 +54:40:20.3: 13.00 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.18
Forced photometry filter REJECTED candidate at 23:24:29.16 +54:40:20.3: ref_mag=13.16 +/- 0.18 new_mean_mag=12.4207 delta=0.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:30.28 +52:00:34.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:30.28 +52:00:34.9: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:59.88 +56:37:34.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:59.88 +56:37:34.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:59.07 +55:38:49.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:59.07 +55:38:49.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:00.79 +57:24:42.7: 11.44 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:56.19 +52:20:52.9: 12.24 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:00.79 +57:24:42.7: 11.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.03
Forced photometry filter REJECTED candidate at 23:42:00.79 +57:24:42.7: ref_mag=11.30 +/- 0.03 new_mean_mag=12.1658 delta=-0.87 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:10.57 +53:55:06.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:56.19 +52:20:52.9: 12.04 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.06
Forced photometry filter REJECTED candidate at 23:39:56.19 +52:20:52.9: ref_mag=12.14 +/- 0.06 new_mean_mag=12.0358 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:23.53 +57:27:47.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:45.63 +54:00:29.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:10.57 +53:55:06.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:23.53 +57:27:47.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:45.63 +54:00:29.4: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:45.35 +55:45:22.5: 13.47 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:04.20 +53:15:53.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:45.35 +55:45:22.5: 13.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.47 +/- 0.31
Forced photometry filter KEPT candidate at 23:41:45.35 +55:45:22.5: ref_mag=13.47 +/- 0.31 new_mean_mag=12.0797 delta=1.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:29.64 +54:54:32.6: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:04.20 +53:15:53.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:29.64 +54:54:32.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:25.74 +51:54:36.1: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:25.74 +51:54:36.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:50.57 +50:59:28.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:50.57 +50:59:28.9: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:31.06 +56:36:50.3: 12.38 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:56.77 +51:10:34.7: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:31.06 +56:36:50.3: 12.21 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:56.77 +51:10:34.7: 13.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.30 +/- 0.10
Forced photometry filter REJECTED candidate at 23:11:31.06 +56:36:50.3: ref_mag=12.30 +/- 0.10 new_mean_mag=12.2397 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:50.48 +50:30:38.3: 13.53 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:50.48 +50:30:38.3: 13.16 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.18
Forced photometry filter KEPT candidate at 23:44:50.48 +50:30:38.3: ref_mag=13.32 +/- 0.18 new_mean_mag=11.7753 delta=1.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:08.06 +57:09:44.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:08.06 +57:09:44.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:39.57 +52:23:57.9: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:39.57 +52:23:57.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:55.66 +54:58:03.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:55.66 +54:58:03.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:47.84 +56:08:37.0: 13.78 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:47.84 +56:08:37.0: 13.18 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.19
Forced photometry filter KEPT candidate at 00:01:47.84 +56:08:37.0: ref_mag=13.36 +/- 0.19 new_mean_mag=11.8987 delta=1.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:21.36 +51:55:18.8: 12.74 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:21.36 +51:55:18.8: 12.52 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.09
Forced photometry filter KEPT candidate at 23:52:21.36 +51:55:18.8: ref_mag=12.62 +/- 0.09 new_mean_mag=11.6236 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:20.19 +54:55:23.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:20.19 +54:55:23.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:14.13 +55:25:04.5: 12.90 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:14.13 +55:25:04.5: 12.71 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.12
Forced photometry filter KEPT candidate at 23:54:14.13 +55:25:04.5: ref_mag=12.81 +/- 0.12 new_mean_mag=11.8039 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:48.28 +56:54:17.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:48.28 +56:54:17.2: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:30.27 +57:44:07.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:30.27 +57:44:07.9: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:57.53 +51:01:10.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:57.53 +51:01:10.4: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:32.23 +54:50:52.8: 13.01 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:32.23 +54:50:52.8: 12.57 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.14
Forced photometry filter REJECTED candidate at 23:27:32.23 +54:50:52.8: ref_mag=12.72 +/- 0.14 new_mean_mag=11.9792 delta=0.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:02.98 +51:37:26.1: 12.23 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:02.98 +51:37:26.1: 11.90 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.06
Forced photometry filter REJECTED candidate at 23:17:02.98 +51:37:26.1: ref_mag=12.03 +/- 0.06 new_mean_mag=11.9298 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:50.71 +54:41:18.2: 13.37 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:40.06 +55:39:47.3: 12.63 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:50.71 +54:41:18.2: 13.05 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.18
Forced photometry filter KEPT candidate at 23:44:50.71 +54:41:18.2: ref_mag=13.19 +/- 0.18 new_mean_mag=11.7224 delta=1.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:40.06 +55:39:47.3: 12.42 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.08
Forced photometry filter REJECTED candidate at 23:56:40.06 +55:39:47.3: ref_mag=12.52 +/- 0.08 new_mean_mag=11.7038 delta=0.82 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:43.69 +50:56:32.7: 13.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:43.69 +50:56:32.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:33.48 +53:36:16.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:33.48 +53:36:16.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:05.97 +56:05:25.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:05.97 +56:05:25.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:18.69 +56:19:02.6: 13.46 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:18.69 +56:19:02.6: 13.35 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.21
Forced photometry filter KEPT candidate at 23:18:18.69 +56:19:02.6: ref_mag=13.41 +/- 0.21 new_mean_mag=11.7319 delta=1.68 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:46.28 +55:21:51.6: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:46.28 +55:21:51.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:17.89 +54:52:52.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:17.89 +54:52:52.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:15.10 +52:14:45.7: 13.55 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:15.10 +52:14:45.7: 13.09 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.20
Forced photometry filter KEPT candidate at 23:15:15.10 +52:14:45.7: ref_mag=13.26 +/- 0.20 new_mean_mag=11.8076 delta=1.45 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:17.41 +55:07:46.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:47.14 +54:51:25.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:17.41 +55:07:46.7: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:47.14 +54:51:25.6: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:57.26 +55:20:51.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:57.26 +55:20:51.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:07.53 +55:23:54.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:27.44 +55:35:12.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:07.53 +55:23:54.3: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:27.44 +55:35:12.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:53.20 +56:58:22.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:53.20 +56:58:22.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:28.22 +56:13:38.9: 10.58 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:28.22 +56:13:38.9: 10.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:28.22 +56:13:38.9: ref_mag=10.41 +/- 0.01 new_mean_mag=11.3275 delta=-0.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:56.70 +52:27:18.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:56.70 +52:27:18.5: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:57.02 +55:03:50.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:57.02 +55:03:50.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:41.19 +54:16:18.5: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:17.57 +56:46:56.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:41.19 +54:16:18.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:17.57 +56:46:56.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:40.05 +53:54:14.7: 13.24 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:40.05 +53:54:14.7: 13.16 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.14
Forced photometry filter KEPT candidate at 23:58:40.05 +53:54:14.7: ref_mag=13.20 +/- 0.14 new_mean_mag=11.0027 delta=2.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:23.21 +57:13:12.9: 13.62 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:23.21 +57:13:12.9: 13.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.62 +/- 0.32
Forced photometry filter KEPT candidate at 23:28:23.21 +57:13:12.9: ref_mag=13.62 +/- 0.32 new_mean_mag=11.2231 delta=2.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:33.94 +56:44:14.8: 11.78 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:33.94 +56:44:14.8: 11.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.06
Forced photometry filter REJECTED candidate at 23:56:33.94 +56:44:14.8: ref_mag=11.57 +/- 0.06 new_mean_mag=10.9880 delta=0.59 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:41.88 +57:16:03.1: 13.56 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:41.88 +57:16:03.1: 13.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.56 +/- 0.29
Forced photometry filter KEPT candidate at 23:39:41.88 +57:16:03.1: ref_mag=13.56 +/- 0.29 new_mean_mag=11.0680 delta=2.49 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:58.47 +50:16:18.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.21 +54:49:12.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:58.47 +50:16:18.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:41.21 +54:49:12.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:08.84 +53:45:18.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:08.84 +53:45:18.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:02.51 +56:51:40.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:02.51 +56:51:40.2: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:25.84 +49:51:13.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:25.84 +49:51:13.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:26.44 +49:36:03.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:26.44 +49:36:03.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:32.65 +50:40:32.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:32.65 +50:40:32.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:01.62 +54:00:51.3: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:01.62 +54:00:51.3: 13.34 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.27
Forced photometry filter KEPT candidate at 23:22:01.62 +54:00:51.3: ref_mag=13.34 +/- 0.27 new_mean_mag=9.5606 delta=3.78 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:57.79 +55:40:10.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:57.79 +55:40:10.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:03.73 +55:52:05.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:03.73 +55:52:05.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:36.60 +57:23:00.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:36.60 +57:23:00.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.62 +53:20:37.2: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:56.62 +53:20:37.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:38.90 +53:34:20.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:38.90 +53:34:20.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:46.75 +52:18:45.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:46.75 +52:18:45.2: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:36.54 +50:10:57.3: 13.33 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:36.54 +50:10:57.3: 13.04 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.18
Forced photometry filter KEPT candidate at 23:29:36.54 +50:10:57.3: ref_mag=13.17 +/- 0.18 new_mean_mag=11.1773 delta=1.99 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:56.46 +53:10:41.2: 9.65 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:56.46 +53:10:41.2: 9.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.38 +/- 0.01
Forced photometry filter REJECTED candidate at 23:17:56.46 +53:10:41.2: ref_mag=9.38 +/- 0.01 new_mean_mag=11.4163 delta=-2.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.73 +57:05:10.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.73 +57:05:10.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:47.54 +54:34:20.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:47.54 +54:34:20.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:32.25 +55:36:22.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:32.25 +55:36:22.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:47.78 +49:05:02.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:47.78 +49:05:02.6: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.71 +55:18:27.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:13.30 +52:06:49.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.71 +55:18:27.8: 13.51 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.36
Forced photometry filter KEPT candidate at 23:11:51.71 +55:18:27.8: ref_mag=13.51 +/- 0.36 new_mean_mag=11.7736 delta=1.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:13.30 +52:06:49.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:14.58 +53:01:29.6: 9.24 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:14.58 +53:01:29.6: 8.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.10 +/- 0.00
Forced photometry filter REJECTED candidate at 23:24:14.58 +53:01:29.6: ref_mag=9.10 +/- 0.00 new_mean_mag=11.5970 delta=-2.50 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.04 +49:20:10.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:27.64 +55:39:37.5: 13.35 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:28.04 +49:20:10.3: 13.42 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.32
Forced photometry filter KEPT candidate at 23:25:28.04 +49:20:10.3: ref_mag=13.42 +/- 0.32 new_mean_mag=11.7403 delta=1.68 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:27.64 +55:39:37.5: 12.70 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.16
Forced photometry filter KEPT candidate at 00:03:27.64 +55:39:37.5: ref_mag=12.89 +/- 0.16 new_mean_mag=11.4962 delta=1.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:01.74 +56:09:11.5: 12.09 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:01.74 +56:09:11.5: 11.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.05
Forced photometry filter REJECTED candidate at 23:14:01.74 +56:09:11.5: ref_mag=11.92 +/- 0.05 new_mean_mag=12.0081 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:21.35 +55:04:15.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:21.35 +55:04:15.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:28.98 +54:27:12.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:16.93 +54:35:02.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:28.98 +54:27:12.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:16.93 +54:35:02.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:37.76 +55:46:51.4: 12.89 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:14.37 +51:45:06.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:37.76 +55:46:51.4: 12.59 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.11
Forced photometry filter REJECTED candidate at 23:18:37.76 +55:46:51.4: ref_mag=12.72 +/- 0.11 new_mean_mag=11.9440 delta=0.77 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:14.37 +51:45:06.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.02 +51:39:58.4: 13.23 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:24.02 +51:39:58.4: 13.05 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.15
Forced photometry filter KEPT candidate at 23:29:24.02 +51:39:58.4: ref_mag=13.14 +/- 0.15 new_mean_mag=11.7376 delta=1.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.18 +54:02:57.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.18 +54:02:57.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:12.94 +57:36:26.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:12.94 +57:36:26.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:12.79 +54:21:37.3: 11.97 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:53.15 +54:29:06.4: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:12.79 +54:21:37.3: 11.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.06
Forced photometry filter REJECTED candidate at 23:52:12.79 +54:21:37.3: ref_mag=11.89 +/- 0.06 new_mean_mag=11.6377 delta=0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:53.15 +54:29:06.4: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:49.97 +54:40:27.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:49.97 +54:40:27.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:32.31 +49:52:17.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:32.31 +49:52:17.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:37.39 +57:23:26.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:37.39 +57:23:26.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:32.72 +54:34:06.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:32.72 +54:34:06.2: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:18.84 +57:40:50.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:18.84 +57:40:50.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:51.95 +54:55:10.8: 10.92 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:51.95 +54:55:10.8: 10.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.72 +/- 0.02
Forced photometry filter REJECTED candidate at 23:24:51.95 +54:55:10.8: ref_mag=10.72 +/- 0.02 new_mean_mag=11.9993 delta=-1.28 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:37.60 +52:09:11.4: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:37.60 +52:09:11.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:21.34 +53:10:39.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:21.34 +53:10:39.4: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:42.33 +56:38:22.8: 11.63 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:42.33 +56:38:22.8: 11.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.03
Forced photometry filter REJECTED candidate at 00:11:42.33 +56:38:22.8: ref_mag=11.42 +/- 0.03 new_mean_mag=11.7561 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:34.88 +53:01:03.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:34.88 +53:01:03.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:53.99 +52:19:34.6: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:53.99 +52:19:34.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:00.32 +53:01:54.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:29.49 +52:31:58.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:00.32 +53:01:54.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:29.49 +52:31:58.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.84 +51:59:43.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:53.84 +51:59:43.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:00.12 +53:55:31.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:00.12 +53:55:31.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:58.60 +57:32:01.4: 10.55 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:58.60 +57:32:01.4: 10.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.02
Forced photometry filter REJECTED candidate at 00:11:58.60 +57:32:01.4: ref_mag=10.41 +/- 0.02 new_mean_mag=11.8497 delta=-1.44 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:05.23 +57:14:02.8: 11.35 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:05.23 +57:14:02.8: 11.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.03
Forced photometry filter REJECTED candidate at 23:45:05.23 +57:14:02.8: ref_mag=11.18 +/- 0.03 new_mean_mag=12.0637 delta=-0.88 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:28.15 +53:18:12.7: 11.50 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:28.15 +53:18:12.7: 11.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.03
Forced photometry filter REJECTED candidate at 00:01:28.15 +53:18:12.7: ref_mag=11.37 +/- 0.03 new_mean_mag=11.8672 delta=-0.50 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:12.15 +56:29:06.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:11.13 +52:25:59.1: 12.17 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:12.15 +56:29:06.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.47 +54:27:10.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:11.13 +52:25:59.1: 11.88 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.06
Forced photometry filter REJECTED candidate at 00:18:11.13 +52:25:59.1: ref_mag=12.01 +/- 0.06 new_mean_mag=11.7986 delta=0.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:46.47 +54:27:10.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:04.90 +51:12:18.2: 13.24 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:04.90 +51:12:18.2: 13.13 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.18
Forced photometry filter REJECTED candidate at 23:36:04.90 +51:12:18.2: ref_mag=13.19 +/- 0.18 new_mean_mag=12.4265 delta=0.76 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:01.31 +49:55:45.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:01.31 +49:55:45.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:12.03 +50:00:11.7: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:12.03 +50:00:11.7: 13.47 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out219245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25587.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 156s
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: 89s
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Considering the candidate 235413_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235413_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235424_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235424_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235435_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235435_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235443_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235443_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235445_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235445_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235450_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235450_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235451_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235451_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235459_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235459_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235465_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235465_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235470_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235470_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235477_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235477_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:20.52 +54:06:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235478_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235478_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235479_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235479_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235483_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235483_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 235485_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235485_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 235493_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235493_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:25:18.42 +57:45:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235499_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235499_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235503_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235503_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235509_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235509_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235516_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235516_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235518_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235518_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235519_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235519_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235525_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235525_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:11:49.39 +54:49:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235527_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235527_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235528_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235528_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235531_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235531_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:41:57.35 +51:42:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235536_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235536_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:08:36.96 +55:38:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235541_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235541_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235543_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235543_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235544_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235544_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235547_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235547_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235549_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235549_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235554_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235554_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235560_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235560_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235562_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235562_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235563_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235563_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235569_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235569_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235573_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235573_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235579_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235579_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235581_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235581_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235582_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235582_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235583_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235583_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235584_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235584_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:29:32.30 +55:19:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235587_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235587_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235588_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235588_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235591_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235591_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:08:33.54 +56:46:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235609_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235609_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235619_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235619_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:04:21.75 +51:49:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235623_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235623_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235628_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235628_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235639_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235639_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235644_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235644_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235652_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235652_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235658_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235658_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235661_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235661_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235663_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235663_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235666_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235666_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235668_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235668_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:25:16.25 +53:39:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235675_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235675_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235680_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235680_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:29:10.64 +56:40:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235683_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235683_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235685_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235685_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:20:24.83 +53:16:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235687_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235687_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235691_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235691_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235693_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235693_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:26:42.64 +54:33:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235694_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235694_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:57:15.99 +56:30:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235696_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235696_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:56:59.89 +56:44:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235701_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235701_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235706_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235706_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235711_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235711_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 235716_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235716_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235717_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235717_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:14:15.32 +54:02:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235719_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235719_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235720_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235720_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235721_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235721_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235723_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235723_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:31:59.48 +54:22:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235724_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235724_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235730_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235730_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:02.07 +57:11:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235731_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235731_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:51:56.65 +53:07:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235735_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235735_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235742_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235742_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235743_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235743_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235744_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235744_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235745_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 235745_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:46:46.56 +51:02:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235939_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 235939_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236060_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236060_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:13:11.45 +57:10:46.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236120_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236120_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:43:56.62 +56:20:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236145_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236145_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:59:23.84 +50:31:40.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236181_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236181_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:31:20.76 +49:29:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236183_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236183_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:18:49.78 +54:33:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236193_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236193_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:47:14.65 +57:25:44.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236218_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236218_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236231_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236231_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236235_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236235_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236262_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236262_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236337_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236337_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:15:42.62 +54:52:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236346_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236346_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236355_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236355_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:37.77 +54:45:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236384_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236384_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236391_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236391_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:25:46.08 +57:59:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236421_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236421_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236425_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236425_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:16:20.76 +53:35:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236437_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236437_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:23:25.85 +55:49:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236446_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236446_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236448_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236448_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:02:36.46 +55:35:40.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236458_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236458_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:59:07.18 +53:34:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236474_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236474_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236485_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236485_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:13:37.57 +56:24:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236512_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236512_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:57:59.48 +50:26:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236524_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236524_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:43:18.38 +50:54:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236539_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236539_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236545_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236545_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:31:44.03 +55:25:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236555_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236555_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236575_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236575_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:38:44.12 +56:37:48.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236590_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236590_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:56:32.04 +53:44:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236621_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236621_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236628_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236628_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236666_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236666_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:10:29.10 +49:51:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236672_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236672_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236684_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236684_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:21:17.09 +55:55:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236687_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236687_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:58:51.66 +54:42:06.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236697_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236697_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:25:48.77 +57:59:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236719_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236719_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:57:58.48 +50:27:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236756_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236756_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:37:53.22 +50:55:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236760_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236760_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:59:00.28 +53:16:18.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236761_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236761_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:43:15.42 +51:56:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236841_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236841_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:40:53.48 +54:25:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236861_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236861_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:31:40.55 +54:09:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236864_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236864_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:24:57.57 +53:01:59.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236870_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236870_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:56:18.04 +56:10:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236876_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236876_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:12:36.58 +57:12:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236883_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236883_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236888_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236888_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236893_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236893_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236894_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236894_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:38:36.50 +57:11:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236898_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236898_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:47:42.26 +56:51:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236908_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236908_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:08:02.01 +53:40:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236914_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236914_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236916_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236916_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:53:43.26 +56:48:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236921_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236921_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:59.47 +57:36:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236939_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236939_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:13:03.28 +49:56:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236942_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236942_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:20:12.65 +50:06:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236947_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236947_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:51.68 +51:53:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236954_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236954_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236958_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236958_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236964_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236964_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:34:07.90 +51:35:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236966_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 236966_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236976_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236976_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236986_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 236986_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237002_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237002_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237003_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237003_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:20.18 +57:20:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237013_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237013_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:02:27.05 +54:33:03.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237022_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237022_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:55:15.68 +50:14:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237025_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237025_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237026_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237026_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:43:22.25 +55:42:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237031_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237031_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:29:40.17 +57:40:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237038_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237038_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:34.98 +54:04:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237041_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237041_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:00:23.27 +56:50:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237046_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237046_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:14:17.04 +56:52:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237065_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237065_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237072_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237072_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237079_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237079_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:04:15.57 +54:16:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237083_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237083_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:55:07.02 +56:11:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237084_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237084_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237104_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237104_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237112_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237112_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:31:37.50 +56:54:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237142_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237142_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237157_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237157_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:50:23.56 +54:12:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237168_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237168_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237176_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237176_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:47:36.81 +55:14:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237187_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237187_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237203_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237203_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:31.72 +51:13:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237204_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237204_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:14:01.22 +55:16:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237212_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237212_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237213_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237213_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:51:00.02 +54:43:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237221_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237221_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237222_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237222_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:18:54.34 +53:18:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237226_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237226_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:55:33.12 +52:42:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237239_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237239_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237248_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237248_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 237258_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237258_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:22:46.47 +56:26:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237263_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237263_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:54:44.73 +53:43:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237276_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237276_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:45:55.05 +56:56:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237280_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237280_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237282_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237282_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237287_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237287_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 237289_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237289_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:12:53.27 +55:50:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237304_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237304_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237309_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237309_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:07:40.70 +57:11:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237334_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237334_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237340_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237340_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 237345_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237345_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237355_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237355_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:37:56.60 +52:41:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237358_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237358_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:01:49.75 +52:51:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237364_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237364_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
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Considering the candidate 237368_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237368_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237394_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237394_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:30:16.52 +55:41:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237396_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237396_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237402_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237402_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:31:28.84 +56:42:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237427_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237427_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:38:09.42 +57:45:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237442_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237442_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 237485_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237485_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:03:40.85 +53:56:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237492_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237492_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:24:30.33 +53:19:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237511_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237511_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237528_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237528_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:28:35.54 +54:26:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237577_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237577_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237622_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 237622_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237625_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 237625_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219159_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 219159_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:27:11.47 +53:53:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219245_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 219245_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:09:36.45 +51:34:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 179100_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 00:15:50.73 +57:32:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:31.90 +56:34:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46078_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063
The candidate 46078_fd_Cas-04-Q2b1x1_2026-07-14_22-49-35_20.00sec_5.00C_LIGHT_0063 did not pass the final checks
**** FOUND 23:58:25.24 +51:23:23.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 254s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:26:01.31 +49:55:45.8
23:34:30.37 +54:23:52.2
23:37:25.08 +51:16:42.3
23:37:44.91 +53:08:11.5
23:26:13.25 +57:06:48.2
23:44:33.09 +53:02:41.9
23:42:49.01 +51:38:40.2
23:26:09.41 +56:23:37.1
23:20:07.64 +54:31:56.6
23:19:22.11 +53:12:39.3
23:28:30.28 +52:00:34.9
23:34:59.88 +56:37:34.9
23:43:59.07 +55:38:49.6
23:21:10.57 +53:55:06.4
23:14:45.63 +54:00:29.4
23:43:23.53 +57:27:47.9
23:41:45.35 +55:45:22.5
23:28:04.20 +53:15:53.6
23:53:29.64 +54:54:32.6
23:32:25.74 +51:54:36.1
23:37:50.57 +50:59:28.9
23:30:56.77 +51:10:34.7
23:44:50.48 +50:30:38.3
23:23:08.06 +57:09:44.1
23:23:39.57 +52:23:57.9
23:22:55.66 +54:58:03.6
00:01:47.84 +56:08:37.0
23:52:21.36 +51:55:18.8
23:35:20.19 +54:55:23.7
23:54:14.13 +55:25:04.5
23:31:48.28 +56:54:17.2
00:24:30.27 +57:44:07.9
23:28:57.53 +51:01:10.4
23:44:50.71 +54:41:18.2
00:02:43.69 +50:56:32.7
23:28:33.48 +53:36:16.9
00:19:05.97 +56:05:25.5
23:18:18.69 +56:19:02.6
00:01:46.28 +55:21:51.6
23:30:17.89 +54:52:52.2
23:15:15.10 +52:14:45.7
23:17:17.41 +55:07:46.7
23:12:47.14 +54:51:25.6
23:18:57.26 +55:20:51.0
23:11:07.53 +55:23:54.3
23:35:27.44 +55:35:12.0
23:36:53.20 +56:58:22.4
23:15:56.70 +52:27:18.5
00:14:57.02 +55:03:50.7
23:18:41.19 +54:16:18.5
23:22:17.57 +56:46:56.9
23:58:40.05 +53:54:14.7
23:28:23.21 +57:13:12.9
23:39:41.88 +57:16:03.1
23:25:58.47 +50:16:18.4
23:12:41.21 +54:49:12.9
23:13:08.84 +53:45:18.4
23:10:02.51 +56:51:40.2
23:50:25.84 +49:51:13.2
23:27:26.44 +49:36:03.3
23:36:32.65 +50:40:32.9
23:22:01.62 +54:00:51.3
23:20:57.79 +55:40:10.6
23:23:03.73 +55:52:05.7
23:22:36.60 +57:23:00.6
23:18:56.62 +53:20:37.2
23:13:38.90 +53:34:20.0
23:28:46.75 +52:18:45.2
23:29:36.54 +50:10:57.3
23:12:17.73 +57:05:10.2
23:23:47.54 +54:34:20.7
23:19:32.25 +55:36:22.9
23:19:47.78 +49:05:02.6
23:11:51.71 +55:18:27.8
23:23:13.30 +52:06:49.9
23:25:28.04 +49:20:10.3
00:03:27.64 +55:39:37.5
23:13:21.35 +55:04:15.2
23:17:28.98 +54:27:12.1
23:21:16.93 +54:35:02.7
23:42:14.37 +51:45:06.4
23:29:24.02 +51:39:58.4
23:34:08.18 +54:02:57.8
00:11:12.94 +57:36:26.1
23:24:53.15 +54:29:06.4
23:41:49.97 +54:40:27.0
23:30:32.31 +49:52:17.5
23:22:37.39 +57:23:26.7
23:14:32.72 +54:34:06.2
23:56:18.84 +57:40:50.0
23:25:37.60 +52:09:11.4
23:32:21.34 +53:10:39.4
23:24:34.88 +53:01:03.4
23:28:53.99 +52:19:34.6
23:44:00.32 +53:01:54.5
23:17:29.49 +52:31:58.0
00:04:53.84 +51:59:43.8
23:22:00.12 +53:55:31.1
23:31:12.15 +56:29:06.0
23:14:46.47 +54:27:10.7
23:21:12.03 +50:00:11.7
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:34:30.37 +54:23:52.2
23:37:25.08 +51:16:42.3
23:37:44.91 +53:08:11.5
23:26:13.25 +57:06:48.2
23:44:33.09 +53:02:41.9
23:42:49.01 +51:38:40.2
23:26:09.41 +56:23:37.1
23:20:07.64 +54:31:56.6
23:19:22.11 +53:12:39.3
23:28:30.28 +52:00:34.9
23:34:59.88 +56:37:34.9
23:43:59.07 +55:38:49.6
23:21:10.57 +53:55:06.4
23:14:45.63 +54:00:29.4
23:43:23.53 +57:27:47.9
23:41:45.35 +55:45:22.5
23:28:04.20 +53:15:53.6
23:53:29.64 +54:54:32.6
23:32:25.74 +51:54:36.1
23:37:50.57 +50:59:28.9
23:30:56.77 +51:10:34.7
23:44:50.48 +50:30:38.3
23:23:08.06 +57:09:44.1
23:23:39.57 +52:23:57.9
23:22:55.66 +54:58:03.6
00:01:47.84 +56:08:37.0
23:52:21.36 +51:55:18.8
23:35:20.19 +54:55:23.7
23:54:14.13 +55:25:04.5
23:31:48.28 +56:54:17.2
00:24:30.27 +57:44:07.9
23:28:57.53 +51:01:10.4
23:44:50.71 +54:41:18.2
00:02:43.69 +50:56:32.7
23:28:33.48 +53:36:16.9
00:19:05.97 +56:05:25.5
23:18:18.69 +56:19:02.6
00:01:46.28 +55:21:51.6
23:30:17.89 +54:52:52.2
23:15:15.10 +52:14:45.7
23:17:17.41 +55:07:46.7
23:12:47.14 +54:51:25.6
23:18:57.26 +55:20:51.0
23:11:07.53 +55:23:54.3
23:35:27.44 +55:35:12.0
23:36:53.20 +56:58:22.4
23:15:56.70 +52:27:18.5
00:14:57.02 +55:03:50.7
23:18:41.19 +54:16:18.5
23:22:17.57 +56:46:56.9
23:58:40.05 +53:54:14.7
23:28:23.21 +57:13:12.9
23:39:41.88 +57:16:03.1
23:25:58.47 +50:16:18.4
23:12:41.21 +54:49:12.9
23:13:08.84 +53:45:18.4
23:10:02.51 +56:51:40.2
23:50:25.84 +49:51:13.2
23:27:26.44 +49:36:03.3
23:36:32.65 +50:40:32.9
23:22:01.62 +54:00:51.3
23:20:57.79 +55:40:10.6
23:23:03.73 +55:52:05.7
23:22:36.60 +57:23:00.6
23:18:56.62 +53:20:37.2
23:13:38.90 +53:34:20.0
23:28:46.75 +52:18:45.2
23:29:36.54 +50:10:57.3
23:12:17.73 +57:05:10.2
23:23:47.54 +54:34:20.7
23:19:32.25 +55:36:22.9
23:19:47.78 +49:05:02.6
23:11:51.71 +55:18:27.8
23:23:13.30 +52:06:49.9
23:25:28.04 +49:20:10.3
00:03:27.64 +55:39:37.5
23:13:21.35 +55:04:15.2
23:17:28.98 +54:27:12.1
23:21:16.93 +54:35:02.7
23:42:14.37 +51:45:06.4
23:29:24.02 +51:39:58.4
23:34:08.18 +54:02:57.8
00:11:12.94 +57:36:26.1
23:24:53.15 +54:29:06.4
23:41:49.97 +54:40:27.0
23:30:32.31 +49:52:17.5
23:22:37.39 +57:23:26.7
23:14:32.72 +54:34:06.2
23:56:18.84 +57:40:50.0
23:25:37.60 +52:09:11.4
23:32:21.34 +53:10:39.4
23:24:34.88 +53:01:03.4
23:28:53.99 +52:19:34.6
23:44:00.32 +53:01:54.5
23:17:29.49 +52:31:58.0
00:04:53.84 +51:59:43.8
23:22:00.12 +53:55:31.1
23:31:12.15 +56:29:06.0
23:14:46.47 +54:27:10.7
23:26:01.31 +49:55:45.8
23:21:12.03 +50:00:11.7
###################################################################################
23:34:30.37 +54:23:52.2 -- not an asteroid (will add it to exclusion list)
23:37:25.08 +51:16:42.3 -- not an asteroid (will add it to exclusion list)
23:37:44.91 +53:08:11.5 -- not an asteroid (will add it to exclusion list)
23:26:13.25 +57:06:48.2 -- not an asteroid (will add it to exclusion list)
23:44:33.09 +53:02:41.9 -- not an asteroid (will add it to exclusion list)
23:42:49.01 +51:38:40.2 -- not an asteroid (will add it to exclusion list)
23:26:09.41 +56:23:37.1 -- not an asteroid (will add it to exclusion list)
23:20:07.64 +54:31:56.6 -- not an asteroid (will add it to exclusion list)
23:19:22.11 +53:12:39.3 -- not an asteroid (will add it to exclusion list)
23:28:30.28 +52:00:34.9 -- not an asteroid (will add it to exclusion list)
23:34:59.88 +56:37:34.9 -- not an asteroid (will add it to exclusion list)
23:43:59.07 +55:38:49.6 -- not an asteroid (will add it to exclusion list)
23:21:10.57 +53:55:06.4 -- not an asteroid (will add it to exclusion list)
23:14:45.63 +54:00:29.4 -- not an asteroid (will add it to exclusion list)
23:43:23.53 +57:27:47.9 -- not an asteroid (will add it to exclusion list)
23:41:45.35 +55:45:22.5 -- not an asteroid (will add it to exclusion list)
23:28:04.20 +53:15:53.6 -- not an asteroid (will add it to exclusion list)
23:53:29.64 +54:54:32.6 -- not an asteroid (will add it to exclusion list)
23:32:25.74 +51:54:36.1 -- not an asteroid (will add it to exclusion list)
23:37:50.57 +50:59:28.9 -- not an asteroid (will add it to exclusion list)
23:30:56.77 +51:10:34.7 -- not an asteroid (will add it to exclusion list)
23:44:50.48 +50:30:38.3 -- not an asteroid (will add it to exclusion list)
23:23:08.06 +57:09:44.1 -- not an asteroid (will add it to exclusion list)
23:23:39.57 +52:23:57.9 -- not an asteroid (will add it to exclusion list)
23:22:55.66 +54:58:03.6 -- not an asteroid (will add it to exclusion list)
00:01:47.84 +56:08:37.0 -- not an asteroid (will add it to exclusion list)
23:52:21.36 +51:55:18.8 -- not an asteroid (will add it to exclusion list)
23:35:20.19 +54:55:23.7 -- not an asteroid (will add it to exclusion list)
23:54:14.13 +55:25:04.5 -- not an asteroid (will add it to exclusion list)
23:31:48.28 +56:54:17.2 -- not an asteroid (will add it to exclusion list)
00:24:30.27 +57:44:07.9 -- not an asteroid (will add it to exclusion list)
23:28:57.53 +51:01:10.4 -- not an asteroid (will add it to exclusion list)
23:44:50.71 +54:41:18.2 -- not an asteroid (will add it to exclusion list)
00:02:43.69 +50:56:32.7 -- not an asteroid (will add it to exclusion list)
23:28:33.48 +53:36:16.9 -- not an asteroid (will add it to exclusion list)
00:19:05.97 +56:05:25.5 -- not an asteroid (will add it to exclusion list)
23:18:18.69 +56:19:02.6 -- not an asteroid (will add it to exclusion list)
00:01:46.28 +55:21:51.6 -- not an asteroid (will add it to exclusion list)
23:30:17.89 +54:52:52.2 -- not an asteroid (will add it to exclusion list)
23:15:15.10 +52:14:45.7 -- not an asteroid (will add it to exclusion list)
23:17:17.41 +55:07:46.7 -- not an asteroid (will add it to exclusion list)
23:12:47.14 +54:51:25.6 -- not an asteroid (will add it to exclusion list)
23:18:57.26 +55:20:51.0 -- not an asteroid (will add it to exclusion list)
23:11:07.53 +55:23:54.3 -- not an asteroid (will add it to exclusion list)
23:35:27.44 +55:35:12.0 -- not an asteroid (will add it to exclusion list)
23:36:53.20 +56:58:22.4 -- not an asteroid (will add it to exclusion list)
23:15:56.70 +52:27:18.5 -- not an asteroid (will add it to exclusion list)
00:14:57.02 +55:03:50.7 -- not an asteroid (will add it to exclusion list)
23:18:41.19 +54:16:18.5 -- not an asteroid (will add it to exclusion list)
23:22:17.57 +56:46:56.9 -- not an asteroid (will add it to exclusion list)
23:58:40.05 +53:54:14.7 -- not an asteroid (will add it to exclusion list)
23:28:23.21 +57:13:12.9 -- not an asteroid (will add it to exclusion list)
23:39:41.88 +57:16:03.1 -- not an asteroid (will add it to exclusion list)
23:25:58.47 +50:16:18.4 -- not an asteroid (will add it to exclusion list)
23:12:41.21 +54:49:12.9 -- not an asteroid (will add it to exclusion list)
23:13:08.84 +53:45:18.4 -- not an asteroid (will add it to exclusion list)
23:10:02.51 +56:51:40.2 -- not an asteroid (will add it to exclusion list)
23:50:25.84 +49:51:13.2 -- not an asteroid (will add it to exclusion list)
23:27:26.44 +49:36:03.3 -- not an asteroid (will add it to exclusion list)
23:36:32.65 +50:40:32.9 -- not an asteroid (will add it to exclusion list)
23:22:01.62 +54:00:51.3 -- not an asteroid (will add it to exclusion list)
23:20:57.79 +55:40:10.6 -- not an asteroid (will add it to exclusion list)
23:23:03.73 +55:52:05.7 -- not an asteroid (will add it to exclusion list)
23:22:36.60 +57:23:00.6 -- not an asteroid (will add it to exclusion list)
23:18:56.62 +53:20:37.2 -- not an asteroid (will add it to exclusion list)
23:13:38.90 +53:34:20.0 -- not an asteroid (will add it to exclusion list)
23:28:46.75 +52:18:45.2 -- not an asteroid (will add it to exclusion list)
23:29:36.54 +50:10:57.3 -- not an asteroid (will add it to exclusion list)
23:12:17.73 +57:05:10.2 -- not an asteroid (will add it to exclusion list)
23:23:47.54 +54:34:20.7 -- not an asteroid (will add it to exclusion list)
23:19:32.25 +55:36:22.9 -- not an asteroid (will add it to exclusion list)
23:19:47.78 +49:05:02.6 -- not an asteroid (will add it to exclusion list)
23:11:51.71 +55:18:27.8 -- not an asteroid (will add it to exclusion list)
23:23:13.30 +52:06:49.9 -- not an asteroid (will add it to exclusion list)
23:25:28.04 +49:20:10.3 -- not an asteroid (will add it to exclusion list)
00:03:27.64 +55:39:37.5 -- not an asteroid (will add it to exclusion list)
23:13:21.35 +55:04:15.2 -- not an asteroid (will add it to exclusion list)
23:17:28.98 +54:27:12.1 -- not an asteroid (will add it to exclusion list)
23:21:16.93 +54:35:02.7 -- not an asteroid (will add it to exclusion list)
23:42:14.37 +51:45:06.4 -- not an asteroid (will add it to exclusion list)
23:29:24.02 +51:39:58.4 -- not an asteroid (will add it to exclusion list)
23:34:08.18 +54:02:57.8 -- not an asteroid (will add it to exclusion list)
00:11:12.94 +57:36:26.1 -- not an asteroid (will add it to exclusion list)
23:24:53.15 +54:29:06.4 -- not an asteroid (will add it to exclusion list)
23:41:49.97 +54:40:27.0 -- not an asteroid (will add it to exclusion list)
23:30:32.31 +49:52:17.5 -- not an asteroid (will add it to exclusion list)
23:22:37.39 +57:23:26.7 -- not an asteroid (will add it to exclusion list)
23:14:32.72 +54:34:06.2 -- not an asteroid (will add it to exclusion list)
23:56:18.84 +57:40:50.0 -- not an asteroid (will add it to exclusion list)
23:25:37.60 +52:09:11.4 -- not an asteroid (will add it to exclusion list)
23:32:21.34 +53:10:39.4 -- not an asteroid (will add it to exclusion list)
23:24:34.88 +53:01:03.4 -- not an asteroid (will add it to exclusion list)
23:28:53.99 +52:19:34.6 -- not an asteroid (will add it to exclusion list)
23:44:00.32 +53:01:54.5 -- not an asteroid (will add it to exclusion list)
23:17:29.49 +52:31:58.0 -- not an asteroid (will add it to exclusion list)
00:04:53.84 +51:59:43.8 -- not an asteroid (will add it to exclusion list)
23:22:00.12 +53:55:31.1 -- not an asteroid (will add it to exclusion list)
23:31:12.15 +56:29:06.0 -- not an asteroid (will add it to exclusion list)
23:14:46.47 +54:27:10.7 -- not an asteroid (will add it to exclusion list)
23:26:01.31 +49:55:45.8 -- not an asteroid (will add it to exclusion list)
23:21:12.03 +50:00:11.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:46.28 +55:21:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:47.84 +56:08:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:43.69 +50:56:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:27.64 +55:39:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:53.84 +51:59:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:12.94 +57:36:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:57.02 +55:03:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:05.97 +56:05:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:30.27 +57:44:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:02.51 +56:51:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:07.53 +55:23:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:51.71 +55:18:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:17.73 +57:05:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:41.21 +54:49:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:47.14 +54:51:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:08.84 +53:45:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:21.35 +55:04:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:38.90 +53:34:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:32.72 +54:34:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:45.63 +54:00:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:46.47 +54:27:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:15.10 +52:14:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:56.70 +52:27:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:17.41 +55:07:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:28.98 +54:27:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:29.49 +52:31:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:18.69 +56:19:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:41.19 +54:16:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.62 +53:20:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:57.26 +55:20:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:22.11 +53:12:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:32.25 +55:36:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:47.78 +49:05:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:07.64 +54:31:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:57.79 +55:40:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:10.57 +53:55:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:12.03 +50:00:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:16.93 +54:35:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:00.12 +53:55:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:01.62 +54:00:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:17.57 +56:46:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:36.60 +57:23:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:37.39 +57:23:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:55.66 +54:58:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:03.73 +55:52:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:08.06 +57:09:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:13.30 +52:06:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:39.57 +52:23:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:47.54 +54:34:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:34.88 +53:01:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:53.15 +54:29:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:28.04 +49:20:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:37.60 +52:09:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:58.47 +50:16:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:01.31 +49:55:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:09.41 +56:23:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:13.25 +57:06:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:26.44 +49:36:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:04.20 +53:15:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:23.21 +57:13:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:30.28 +52:00:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:33.48 +53:36:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:46.75 +52:18:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:53.99 +52:19:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:57.53 +51:01:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:24.02 +51:39:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:36.54 +50:10:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:17.89 +54:52:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:32.31 +49:52:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:56.77 +51:10:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:12.15 +56:29:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:48.28 +56:54:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:21.34 +53:10:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:25.74 +51:54:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:08.18 +54:02:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:30.37 +54:23:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:59.88 +56:37:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:20.19 +54:55:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:27.44 +55:35:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:32.65 +50:40:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:53.20 +56:58:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:25.08 +51:16:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:44.91 +53:08:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:50.57 +50:59:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:41.88 +57:16:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:45.35 +55:45:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:49.97 +54:40:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:14.37 +51:45:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:49.01 +51:38:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:23.53 +57:27:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:59.07 +55:38:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:00.32 +53:01:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:33.09 +53:02:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:50.48 +50:30:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:50.71 +54:41:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:25.84 +49:51:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:21.36 +51:55:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:29.64 +54:54:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:14.13 +55:25:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:18.84 +57:40:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:40.05 +53:54:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:01:46.28 +55:21:51.6 -- a known variable star
00:01:47.84 +56:08:37.0 -- not a known variable star
00:02:43.69 +50:56:32.7 -- a known variable star
00:03:27.64 +55:39:37.5 -- not a known variable star
00:04:53.84 +51:59:43.8 -- not a known variable star
00:11:12.94 +57:36:26.1 -- not a known variable star
00:14:57.02 +55:03:50.7 -- not a known variable star
00:19:05.97 +56:05:25.5 -- not a known variable star
00:24:30.27 +57:44:07.9 -- not a known variable star
23:10:02.51 +56:51:40.2 -- not a known variable star
23:11:07.53 +55:23:54.3 -- not a known variable star
23:11:51.71 +55:18:27.8 -- a known variable star
23:12:17.73 +57:05:10.2 -- not a known variable star
23:12:41.21 +54:49:12.9 -- not a known variable star
23:12:47.14 +54:51:25.6 -- not a known variable star
23:13:08.84 +53:45:18.4 -- a known variable star
23:13:21.35 +55:04:15.2 -- not a known variable star
23:13:38.90 +53:34:20.0 -- not a known variable star
23:14:32.72 +54:34:06.2 -- not a known variable star
23:14:45.63 +54:00:29.4 -- a known variable star
23:14:46.47 +54:27:10.7 -- not a known variable star
23:15:15.10 +52:14:45.7 -- not a known variable star
23:15:56.70 +52:27:18.5 -- not a known variable star
23:17:17.41 +55:07:46.7 -- not a known variable star
23:17:28.98 +54:27:12.1 -- not a known variable star
23:17:29.49 +52:31:58.0 -- not a known variable star
23:18:18.69 +56:19:02.6 -- not a known variable star
23:18:41.19 +54:16:18.5 -- not a known variable star
23:18:56.62 +53:20:37.2 -- a known variable star
23:18:57.26 +55:20:51.0 -- not a known variable star
23:19:22.11 +53:12:39.3 -- not a known variable star
23:19:32.25 +55:36:22.9 -- not a known variable star
23:19:47.78 +49:05:02.6 -- not a known variable star
23:20:07.64 +54:31:56.6 -- not a known variable star
23:20:57.79 +55:40:10.6 -- a known variable star
23:21:10.57 +53:55:06.4 -- not a known variable star
23:21:12.03 +50:00:11.7 -- a known variable star
23:21:16.93 +54:35:02.7 -- not a known variable star
23:22:00.12 +53:55:31.1 -- not a known variable star
23:22:01.62 +54:00:51.3 -- not a known variable star
23:22:17.57 +56:46:56.9 -- a known variable star
23:22:36.60 +57:23:00.6 -- not a known variable star
23:22:37.39 +57:23:26.7 -- not a known variable star
23:22:55.66 +54:58:03.6 -- a known variable star
23:23:03.73 +55:52:05.7 -- not a known variable star
23:23:08.06 +57:09:44.1 -- a known variable star
23:23:13.30 +52:06:49.9 -- not a known variable star
23:23:39.57 +52:23:57.9 -- not a known variable star
23:23:47.54 +54:34:20.7 -- a known variable star
23:24:34.88 +53:01:03.4 -- not a known variable star
23:24:53.15 +54:29:06.4 -- not a known variable star
23:25:28.04 +49:20:10.3 -- not a known variable star
23:25:37.60 +52:09:11.4 -- not a known variable star
23:25:58.47 +50:16:18.4 -- not a known variable star
23:26:01.31 +49:55:45.8 -- a known variable star
23:26:09.41 +56:23:37.1 -- not a known variable star
23:26:13.25 +57:06:48.2 -- not a known variable star
23:27:26.44 +49:36:03.3 -- a known variable star
23:28:04.20 +53:15:53.6 -- not a known variable star
23:28:23.21 +57:13:12.9 -- not a known variable star
23:28:30.28 +52:00:34.9 -- not a known variable star
23:28:33.48 +53:36:16.9 -- not a known variable star
23:28:46.75 +52:18:45.2 -- not a known variable star
23:28:53.99 +52:19:34.6 -- not a known variable star
23:28:57.53 +51:01:10.4 -- not a known variable star
23:29:24.02 +51:39:58.4 -- not a known variable star
23:29:36.54 +50:10:57.3 -- not a known variable star
23:30:17.89 +54:52:52.2 -- not a known variable star
23:30:32.31 +49:52:17.5 -- not a known variable star
23:30:56.77 +51:10:34.7 -- not a known variable star
23:31:12.15 +56:29:06.0 -- a known variable star
23:31:48.28 +56:54:17.2 -- not a known variable star
23:32:21.34 +53:10:39.4 -- not a known variable star
23:32:25.74 +51:54:36.1 -- a known variable star
23:34:08.18 +54:02:57.8 -- a known variable star
23:34:30.37 +54:23:52.2 -- not a known variable star
23:34:59.88 +56:37:34.9 -- not a known variable star
23:35:20.19 +54:55:23.7 -- not a known variable star
23:35:27.44 +55:35:12.0 -- not a known variable star
23:36:32.65 +50:40:32.9 -- not a known variable star
23:36:53.20 +56:58:22.4 -- a known variable star
23:37:25.08 +51:16:42.3 -- not a known variable star
23:37:44.91 +53:08:11.5 -- not a known variable star
23:37:50.57 +50:59:28.9 -- not a known variable star
23:39:41.88 +57:16:03.1 -- a known variable star
23:41:45.35 +55:45:22.5 -- not a known variable star
23:41:49.97 +54:40:27.0 -- not a known variable star
23:42:14.37 +51:45:06.4 -- not a known variable star
23:42:49.01 +51:38:40.2 -- a known variable star
23:43:23.53 +57:27:47.9 -- a known variable star
23:43:59.07 +55:38:49.6 -- not a known variable star
23:44:00.32 +53:01:54.5 -- not a known variable star
23:44:33.09 +53:02:41.9 -- not a known variable star
23:44:50.48 +50:30:38.3 -- a known variable star
23:44:50.71 +54:41:18.2 -- a known variable star
23:50:25.84 +49:51:13.2 -- not a known variable star
23:52:21.36 +51:55:18.8 -- not a known variable star
23:53:29.64 +54:54:32.6 -- not a known variable star
23:54:14.13 +55:25:04.5 -- a known variable star
23:56:18.84 +57:40:50.0 -- not a known variable star
23:58:40.05 +53:54:14.7 -- not a known variable star
Found 77 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
101 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 101 (excluding asteroids and hot pixels, 77 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)2461236.65868008 -observatory V36
07:19:26.57 +17:12:21.5 Mercury (5.2mag)
10:31:31.37 +10:31:51.9 Venus (-4.1mag)
04:38:25.39 +21:59:00.1 Mars (1.3mag)
08:21:03.01 +19:57:30.0 Jupiter (-1.8mag)
00:56:18.38 +03:21:53.9 Saturn (0.7mag)
04:08:07.79 +20:47:28.1 Uranus (5.8mag)
00:16:58.81 +00:20:07.4 Neptune (7.7mag)
20:30:28.09 -23:20:07.5 Pluto (14.4mag)
08:19:45.16 +21:08:59.8 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 361 Jul 15 00:17 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461236.65868008:
08:20:59.84 +19:57:43.6 Io (6.1mag)
08:21:11.41 +19:56:57.7 Europa (6.3mag)
08:20:53.41 +19:58:10.2 Ganymede (5.6mag)
08:20:48.32 +19:58:21.7 Callisto (6.8mag)
08:19:21.58 +19:43:45.1 Himalia (15.7mag)
08:21:04.76 +19:57:23.8 Thebe (16.6mag)
08:18:42.29 +19:47:09.1 Elara (17.7mag)
08:24:43.81 +19:49:06.0 Pasiphae (17.8mag)
08:25:44.22 +20:03:17.5 Carme (19.0mag)
00:56:28.03 +03:21:28.9 Titan (8.5mag)
00:56:13.43 +03:21:51.1 Rhea (9.8mag)
00:55:43.84 +03:20:11.0 Iapetus (11.2mag)
00:56:07.60 +03:22:15.7 Hyperion (14.5mag)
00:56:12.69 +03:18:25.6 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 15 00:17 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461236.65868008:
17:53:52.59 -31:54:12.5 JWST
13:35:57.38 +58:12:55.6 Chandra
08:41:51.01 -48:29:11.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 15 00:17 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461236.65868008 -observatory V36
02:43:02.46 +14:59:27.1 17.9mag P/1996 R2 (Lagerkvist)
18:14:20.38 -34:29:01.4 13.8mag P/2010 H2 (Vales)
06:30:28.68 -68:13:19.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:27.69 +32:31:47.0 17.6mag C/2017 K2 (PANSTARRS)
02:13:28.68 +16:47:53.3 15.6mag P/2021 N1 (ZTF)
22:56:33.73 +32:15:44.6 17.3mag C/2022 E2 (ATLAS)
06:17:51.28 +26:52:51.2 16.7mag C/2022 N2 (PANSTARRS)
09:59:43.46 +29:33:54.6 16.9mag C/2022 QE78 (ATLAS)
09:12:51.07 +05:05:08.9 17.9mag C/2022 R6 (PANSTARRS)
18:04:20.21 +21:05:51.0 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:11.30 -11:30:10.3 17.7mag P/2023 B1 (PANSTARRS)
21:43:18.46 +67:33:46.3 17.8mag C/2023 H5 (Lemmon)
16:21:42.45 -10:34:41.5 14.0mag C/2023 R1 (PANSTARRS)
08:09:03.44 +65:58:17.7 17.9mag C/2024 A1 (ATLAS)
07:39:03.90 +30:14:40.8 14.8mag C/2024 E1 (Wierzchos)
15:14:06.16 +15:26:36.2 17.6mag C/2024 G6 (ATLAS)
19:35:06.87 +40:17:32.9 13.8mag C/2024 J3 (ATLAS)
21:42:27.07 +46:42:26.0 17.8mag C/2024 R4 (PANSTARRS)
04:54:08.99 -13:35:17.1 15.7mag C/2024 T5 (ATLAS)
06:38:31.08 +28:16:02.9 18.0mag C/2025 J1 (Borisov)
07:17:38.19 -13:19:44.6 16.7mag C/2025 R3 (PANSTARRS)
10:01:44.14 +22:13:29.9 17.6mag C/2025 V2 (Rankin)
12:46:18.47 +03:43:29.0 17.1mag C/2025 Y1 (ATLAS)
16:38:48.66 +79:10:02.4 17.3mag C/2026 A2 (Bok)
02:51:12.20 +45:26:33.6 16.8mag C/2026 B2 (Sun-Gao)
11:28:38.39 +05:22:15.7 17.0mag A/2026 E1
21:26:30.45 -16:51:44.8 7.1mag 10P/Tempel
11:15:45.18 -02:05:55.1 16.2mag 29P/Schwassmann-Wachmann
04:07:03.87 +30:04:15.5 17.9mag 47P/Ashbrook-Jackson
10:18:06.45 +12:28:30.2 17.1mag 63P/Wild
00:50:19.38 -05:03:05.6 15.5mag 65P/Gunn
04:39:00.56 +20:24:30.6 13.7mag 78P/Gehrels
02:29:58.29 +11:15:20.7 16.3mag 88P/Howell
06:49:45.17 +30:13:28.5 15.7mag 93P/Lovas
04:36:39.96 +31:17:06.3 16.7mag 114P/Wiseman-Skiff
08:20:26.41 +30:09:04.9 15.2mag 123P/West-Hartley
10:57:07.73 -00:45:53.1 16.8mag 124P/Mrkos
04:59:25.97 +20:56:29.8 16.2mag 128P/Shoemaker-Holt
05:45:17.58 +19:39:51.9 17.8mag 131P/Mueller
00:02:44.10 +03:06:39.0 17.9mag 139P/Vaisala-Oterma
07:30:57.90 +15:57:53.3 16.1mag 141P-D/Machholz
03:18:45.45 -20:43:02.6 15.2mag 161P/Hartley-IRAS
05:50:23.89 +34:56:04.7 15.4mag 162P/SidingSpring
18:50:43.33 +18:12:34.6 14.3mag 169P/NEAT
01:52:24.34 +08:06:51.8 17.7mag 220P/McNaught
16:35:31.67 -08:35:23.3 17.1mag 235P/LINEAR
08:55:22.79 +32:50:51.9 18.0mag 240P/NEAT
20:39:51.43 -50:34:30.3 17.8mag 259P/Garradd
02:12:48.44 +14:20:33.5 15.6mag 260P/McNaught
05:51:50.65 +37:11:59.7 17.4mag 295P/LINEAR
15:06:28.66 +05:37:14.0 17.6mag 391P/Kowalski
08:38:55.90 +19:28:44.3 17.9mag 450P/LONEOS
07:59:17.74 +38:48:54.5 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 15 00:17 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 15 00:17 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 15 00:17 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:49:23.723 -15:30:28.94 AT 2026ubs 2026-07-07.41 23.1172
22:47:25.707 -13:21:20.99 AT 2026ubr 2026-07-07.42 22.9851
22:48:27.713 -14:51:00.69 AT 2026ubq 2026-07-07.41 23.5158
22:55:15.603 -17:20:52.24 AT 2026ubp 2026-07-07.41 22.73
00:01:17.781 -03:06:59.77 AT 2026ubo 2026-06-30.36 21.0986
23:48:53.692 +00:34:05.28 AT 2026ubn 2026-06-30.37 21.2974
23:55:47.866 +01:29:21.94 AT 2026ubm 2026-06-30.37 22.7418
23:56:07.829 -00:07:55.59 AT 2026ubl 2026-06-30.36 22.5755
22:50:20.382 -04:24:01.18 AT 2026ubk 2026-06-30.33 21.8405
23:52:09.876 +01:40:51.93 AT 2026ubj 2026-06-30.37 22.5344
23:48:54.336 +01:46:33.67 AT 2026ubi 2026-06-30.37 22.1609
22:50:27.464 -01:58:53.77 AT 2026ubh 2026-06-30.33 21.7659
22:58:59.868 -08:03:37.23 AT 2026ubg 2026-06-30.38 21.6329
23:49:24.946 +01:58:51.32 AT 2026ubf 2026-06-29.44 22.2202
23:59:56.195 -03:44:57.39 AT 2026ube 2026-06-28.41 20.5542
00:00:50.637 -03:46:47.18 AT 2026ubd 2026-06-28.41 21.298
23:45:12.710 +02:24:00.98 AT 2026ubc 2026-06-28.41 22.0341
20:22:20.949 -12:12:52.91 AT 2026ubb 2026-06-27.32 22.8472
22:57:14.411 -03:45:30.21 AT 2026uba 2026-06-27.38 22.8688
21:41:33.046 -11:26:41.30 AT 2026uaz 2026-06-27.33 22.6995
-rw-r--r-- 1 apache apache 30K Jul 15 00:17 tns_transients_list.txt
