DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 SN 1987A 83.8361 -69.2786 83.928024 -69.308301 307.518784 -86.433209 279.71542477 -31.94667609 132.5904 53677.835775463 2005-11-03 20:03:31 53678.3475 2005-11-04 08:20:24 500006010 36.7863 40 36.7863 36.7863 36.7863 36.7863 2 2 2 2 1 0 0 32.9198 32.9198 44.1661 1 PROCESSED 57527.9193518518 2016-05-19 22:03:52 54247 2007-05-27 00:00:00 54037.1281481482 2006-10-29 03:04:32 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001028 SN1987A is providing us with a unique opportunity to study the supernova explosion itself and the very early phase of the supernova-remnants evolution. The supernova blast wave has started to strike the inner circumstellar ring. The neutrino flash observed at the time of explosion implies the formation of a neutron star, but no evidence of this has been detected yet. We propose to observe SN1987A for 40 ksec with Suzaku HXD and XIS. Our first goal is the search for a periodic hard signal from the putative pulsar. We also want to study the collision of the supernova blast wave with the inner ring. In order to follow the temporal evolution of the shock, we propose to observe the source with Suzaku in the early phase of the SWG PV-phase as a reference for further studies. GALACTIC DIFFUSE EMISSION 5 A GUENTHER HASINGER JAP 0 SWG SUZAKU OBSERVATION OF SN1987A : SEARCH FOR PULSAR EMISSION AND STUDY OF A NEWBORN SNR N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500006010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '500006010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏