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 CTB1_NE 0.2869 62.6043 359.6465 62.325973 37.675416 54.459267 117.18345572 0.29518062 253.7193 55923.0281134259 2011-12-28 00:40:29 55924.1251736111 2011-12-29 03:00:15 506035010 52.666 50 52.666 52.666 0 52.666 2 2 0 2 1 0 0 48.3108 48.3108 94.7759 3 PROCESSED 57604.2722569444 2016-08-04 06:32:03 56313 2013-01-21 00:00:00 55972.6734490741 2012-02-15 16:09:46 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060086 CTB 1 is an old (9 - 44 thousand years) galactic supernova remnant (SNR). The ASCA observation of CTB 1 suggested a hard X-ray emission in the 3 - 10 keV band. The hard emission may be originated in synchrotron radiation (non-thermal) or in thermal bremsstrahlung (kT ~ 3 keV). In the case of the non-thermal origin, the old SNR still accelerate electrons up to 100 TeV. On the other hand, the thermal origin indicates that very hot plasma is still kept in such an old SNR. In order to clean up the nature of the hard emission which would give a large impact for the mechanism of particle acceleration and SNR evolution, we propose the Suzaku observation of CTB 1. GALACTIC DIFFUSE EMISSION 5 C SHINYA NAKASHIMA JAP 6 AO6 NON-THERMAL EMISSION FROM THE MOST ANCIENT SUPERNOVA REMNANT XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506035010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506035010'

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