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 XMMU 2235.3-2557 338.8435 -25.9657 338.152793 -26.224773 330.62189 -15.821353 27.27021923 -59.64080614 244.5944 55878.6378125 2011-11-13 15:18:27 55881.5577777778 2011-11-16 13:23:12 806013010 101.1227 100 101.1227 101.1227 0 101.1227 2 2 0 2 1 0 0 90.6244 90.6244 252.2417 4 PROCESSED 57603.8656481482 2016-08-03 20:46:32 56257 2012-11-26 00:00:00 55890.7014583333 2011-11-25 16:50:06 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060038 Galaxy clusters at high redshift are useful as a cosmological probe that have a potential to constrain the inflation theory via its mass function. A massive cluster, XMMU 2235.3-2557 found at z=1.4 is especially important because the presence itself should be quite rare if the standard theory with the Gaussian random field is correct. However, there can be a lot of systematic errors of the mass estimates, that is, the temperature measurement of the cluster. Hence, we propose an independent measurement of X-ray spectroscopic temperature by SUZAKU. EXTRAGALACTIC DIFFUSE SOURCES 8 C HAJIME KAWAHARA JAP 6 AO6 TEMPERATURE MEASUREMENT OF A MASSIVE HIGH-Z CLUSTER XMMU 2235.3-2557 BY SUZAKU XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806013010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '806013010'

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