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 A548W 86.2487 -25.8437 85.742711 -25.86316 84.832695 -49.218426 230.35478522 -25.32458233 240.9996 56337.0028819444 2013-02-14 00:04:09 56339.3300462963 2013-02-16 07:55:16 807033010 99.3707 100 99.3707 99.3707 0 99.3707 2 2 0 2 1 0 0 85.3446 85.3446 201.0437 2 PROCESSED 57610.6626041667 2016-08-10 15:54:09 56738 2014-03-22 00:00:00 56372.6069444445 2013-03-21 14:34:00 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070085 Abell 548 west is a near-by (z=0.0424) poor cluster with an X-ray temperature of 3.4 keV. It has two bright radio relic emission located to the north (Feretti et al. 2006), and a candidate shock-front located near the relics (Solovyeva et al. 2008). The cluster X-ray luminosity is more than an order of magnitude dimmer when plotted in the kT-Lx relation. Combined with its too high galaxy velocity dispersion, we consider this target as a critical merger of two group-sized systems, which is a very rare case in our vicinity. Using Suzaku, we will parametrize the low surface brightness candidate shock region, to identify the temperature jump, which cannot be detected with XMM. We will also investigate the IC emission from the relics to measure the lower limit of its magnetic field. EXTRAGALACTIC DIFFUSE SOURCES 8 C KAZUHIRO NAKAZAWA JAP 7 AO7 SUZAKU OBSERVATION OF A MERGING GROUP CANDIDATE ABELL 548 WEST XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807033010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '807033010'

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