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 ANTLIA CLUSTER 157.5092 -35.3277 156.944615 -35.070958 175.726148 -40.891834 272.94647188 19.18131972 90.0004 54423.2458796296 2007-11-19 05:54:04 54425.0211111111 2007-11-21 00:30:24 802035010 65.9528 60 65.9608 65.9608 0 65.9528 2 2 0 2 1 0 0 58.1064 58.1064 153.3638 2 PROCESSED 57540.5835185185 2016-06-01 14:00:16 54801 2008-12-01 00:00:00 54433.3905092593 2007-11-29 09:22:20 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020101 Suzaku observation of the non-cD cluster Abell 1060 shows that temperature of intra-cluster medium (ICM) increases toward the center. This phenomenon is exact opposite of that of giant cD clusters, in which temperature of the ICM decreases toward the center. To explain this observation, we have proposed that galaxies moving through the ICM interact magnetohydrodynamically with the ICM. This scenario implies that the galaxies have lost some part of their kinetic energies, while the ICM received the released energies. As a result, the ICM have been efficiently heated near the center in which galaxy number density is high. To strengthen our scenario, we propose to observation and study temperature map of the Antlia cluster which is another non-cD, relaxed, and nearby (z=0.0087) cluster. EXTRAGALACTIC DIFFUSE SOURCES 8 C TAKAO KITAGUCHI JAP 2 AO2 SUZAKU OBSERVATION OF NON-CD ANTLIA CLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802035010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802035010'

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