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 A1674_SW 195.6324 67.4673 195.171121 67.735617 143.543166 62.683089 121.29194244 49.62561755 325.0183 56802.7378472222 2014-05-25 17:42:30 56804.2224537037 2014-05-27 05:20:20 809042040 6.3772 40 6.3772 90.8498 0 6.3772 3 2 0 2 1 0 0 71.0768 71.0768 103.0788 1 PROCESSED 57615.185787037 2016-08-15 04:27:32 57626 2016-08-26 00:00:00 56818.7191203704 2014-06-10 17:15:32 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090114 A1674 is a nearby cluster of galaxies, cataloged as richness class 3. Regardless of this extreme richness, its X-ray luminosity is as low as 5e43 erg/s. Our Suzaku AO1 observation revealed that A1674 consists of at least two clusters, one at z~0.2 and the other at z~0.1. Moreover, excess hard X-ray emission was detected with an intensity exceeding the 90% confidence range of the NXB modeling uncertainty. We aim to confirm this hard X-ray emission and to localize that component (really diffuse or point-like) by performing 4 pointings during the AO9 phase. EXTRAGALACTIC DIFFUSE SOURCES 8 B KIYOSHI HAYASHIDA JAP 9 AO9 HARD X-RAY EMISSION IN THE CLUSTER OF GALAXIES A1674 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/809042040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '809042040'

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