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 FESI2 313.183 30.3797 312.661298 30.190122 327.500793 45.583083 73.99193661 -9.03499466 225.2405 55174.9860300926 2009-12-09 23:39:53 55175.7904398148 2009-12-10 18:58:14 504018010 34.5904 34 34.5904 34.5904 0 34.5904 2 2 0 2 1 0 0 30.318 30.318 69.4939 0 PROCESSED 57549.7573032407 2016-06-10 18:10:31 55555 2010-12-25 00:00:00 55189.1622916667 2009-12-24 03:53:42 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040007 The Cygnus Loop is a middle-aged (10,000 yr) supernova remnant. Our past observations have revealed the complex structure of the Loop. We found the abundance inhomogeneity at the edge of the shell, suggesting the existence of the non-thermal component. We also found the blowout region at the center of the Loop. Also, we found the asymmetry of the ejecta distributions, suggesting the asymmetric supernova explosion. Then, our purposes of this observation are summarized in the following three points: 1. To clarify the origin of the abundance inhomogeneity from the shell regions. 2. To determine the accurate structure of the blowout region we found. 3. To investigate the distributions of the heavy elements derived from the hot ejecta component. We propose the 410ks observations in total. GALACTIC DIFFUSE EMISSION 5 B HIROSHI TSUNEMI JAP 4 AO4 OBSERVATION OF THE CYGNUS LOOP WITH THE SUZAKU XIS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504018010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504018010'

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