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 NGC 1553 64.0253 -55.7788 63.753175 -55.901382 28.715493 -73.694617 265.63371114 -43.7014546 176.9406 54429.7042939815 2007-11-25 16:54:11 54431.9029976852 2007-11-27 21:40:19 802050010 98.7222 95 98.7222 98.7222 0 98.7222 2 2 0 2 1 0 0 87.7903 87.7903 189.9159 2 PROCESSED 57540.6454976852 2016-06-01 15:29:31 54806 2008-12-06 00:00:00 54438.4258101852 2007-12-04 10:13:10 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021401 As driving engines of metal enrichment, early-type galaxies provide vital laboratories to investigate how it operates. In our Chandra survey of galaxies, we found solar ISM abundances (Zfe), similar to the stars and implying enrichment homology from clusters to moderate-Lx galaxies. The only outlier was NGC1553, for which we found a tantalizing hint of very subsolar Zfe, inconsistent with simple models. Unlike other galaxies with recent reports of low Zfe, NGC1553 has a bright gas halo, so the results are insensitive to the modelling of unresolved LMXB. We propose an 80ks observation of NGC1553 to measure definitively the ISM abundances of Fe and other crucial diagnostic elements. These data will either confirm enrichment bimodality or provide a vital low-Lx data-point to anchor models. EXTRAGALACTIC DIFFUSE SOURCES 8 C PHILIP HUMPHREY USA 2 AO2 NGC 1553: PROOF OF BIMODAL METAL ENRICHMENT? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802050010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802050010'

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