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 A2256N 256.1941 78.9961 256.949832 79.060716 101.697267 76.992175 111.38046428 31.59001765 219.8042 56234.8690625 2012-11-03 20:51:27 56236.1877083333 2012-11-05 04:30:18 807024010 62.2855 60 62.2855 62.2855 0 62.2855 1 1 0 1 1 0 0 76.5361 76.5361 113.9039 0 PROCESSED 57607.9455555556 2016-08-07 22:41:36 56630 2013-12-04 00:00:00 56260.5238657407 2012-11-29 12:34:22 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070058 We observe outskirts of the famous merging cluster of galaxies A2256 with 4 pointings (60ks for each), and obtain spatial distributions of temperature, electron density, pressure and entropy. In a recent study, the thermal profiles after a merger are thought to be similar to those at cluster formation age. By comparing the spatial distributions of A2256 with those of nearby relaxed clusters, we observationally study the evolution of thermal spatial properties of the ICM in the course of cluster evolution. EXTRAGALACTIC DIFFUSE SOURCES 8 C MADOKA KAWAHARADA JAP 7 AO7 THERMAL EVOLUTION OF THE ICM STUDIED WITH A2256 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807024010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '807024010'

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