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 AWM7 BGD 41.6937 42.4876 40.885444 42.278459 52.542503 25.125109 144.58796377 -15.48250354 257.001 56707.9150810185 2014-02-19 21:57:43 56708.3828587963 2014-02-20 09:11:19 808027010 20.4971 20 20.5011 20.5051 0 20.4971 2 2 0 2 1 0 0 22.116 22.116 40.41 0 PROCESSED 57613.8622106482 2016-08-13 20:41:35 57086 2015-03-05 00:00:00 56720.6154976852 2014-03-04 14:46:19 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080034 We propose to observe AWM 7 cluster at 0.4--0.9 r180 toward northwest and southeast with 4 pointing observations (15 ks x 2+35 ks x 2) and a background field with 20 ks exposure. These directions are between a filament and a void directions and free from systematic errors caused by stray light. The objective is to derive metal-mass-to-light ratios out to the virial radius, and constrain the slope of the initial mass function of stars in early-type galaxies in clusters of galaxies. EXTRAGALACTIC DIFFUSE SOURCES 8 B KYOKO MATSUSHITA JAP 8 AO8 METAL-MASS-TO-LIGHT RATIOS OUT TO THE VIRIAL RADIUS OF THE AWM 7 CLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808027010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808027010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏