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 N1550_CENTER 64.9488 2.4105 64.297881 2.291179 63.464463 -18.753248 191.00239213 -31.81480775 89.9981 54694.185474537 2008-08-16 04:27:05 54696.3009143518 2008-08-18 07:13:19 803017010 83.2702 80 83.7102 83.2702 0 83.7102 2 2 0 2 1 0 0 64.8874 64.8874 182.756 4 PROCESSED 57543.367974537 2016-06-04 08:49:53 55080 2009-09-06 00:00:00 54713.2652546296 2008-09-04 06:21:58 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030070 We propose 80 and 40 ksec observations of the central and 30' offset regions of fossil group, NGC 1550, respectively, to study metal abundance distributions of O to Fe to the ~0.2 times of virial radius. A good energy resolution, and a low and stable background level of the XIS instrument are crucial for this study. A comparison of O to Fe abundance profiles will tell us how metals produced by type Ia and II supernovae have been enriched in the intergalactic space. In addition, a comparison of the metal distributions of the nominal group of galaxies and fossil group will show us how much metal production and diffusion processes differ with system. EXTRAGALACTIC DIFFUSE SOURCES 8 A KOSUKE SATO JAP 3 AO3 OBSERVATIONS OF METAL DISTRIBUTIONS IN FOSSIL GROUP: NGC1550 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803017010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '803017010'

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