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 CYGNUS LOOP 1 313.2462 32.1399 312.732912 31.950084 328.580357 47.179033 75.40840203 -7.96786776 81.7816 55300.7096759259 2010-04-14 17:01:56 55301.0293402778 2010-04-15 00:42:15 505009010 15.9992 13 15.9992 15.9992 0 15.9992 2 2 0 2 1 0 0 12.242 12.242 27.612 0 PROCESSED 57551.2105787037 2016-06-12 05:03:14 55287 2010-04-01 00:00:00 55362.3098726852 2010-06-15 07:26:13 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 050005 The Cygnus Loop is a prototypical middle-aged SNR. Based on the previous observation, the shell shows relatively low temperature with low metal abundance and high non-uniformity in intensity. The interior shows high temperature with high abundance. It also shows the abundance non-uniformity. The inner plasma is the fossil of the progenitor star. The abundance non-uniformity indicates the asymmetric explosion. We propose to observe the rest of the Cygnus Loop for 310ks with three objectives that are tightly correlated to each other. The first is to establish the metal structure that is the key to study the asymmetric explosion. The second is to measure the amount of metal that can determine the progenitor mass. The last one is to search for a compact object such as a neutron star. GALACTIC DIFFUSE EMISSION 5 A HIROSHI TSUNEMI JAP 5 AO5 X-RAY OBSERVATION OF THE CYGNUS LOOP WITH SUZAKU XIS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '505009010'

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